The galaxy presents a complex morphology, appearing as a possible merger or strongly interacting system. Two distinct luminous components are observed, suggesting either two separate galaxies in the process of merging or a single galaxy with a highly disturbed structure. 

The primary component exhibits a relatively smooth, though somewhat elongated, light distribution, lacking clear spiral arm features. The color appears primarily yellow, suggesting an older stellar population with reduced recent star formation.

The secondary component displays a more compact and possibly irregular structure, with a less defined shape. The yellow hue suggests it too has an older population of stars.

A faint bridge of material appears to connect the two components, suggesting a tidal interaction between them. This feature is indicative of gravitational forces acting between the two structures, potentially disrupting their original forms.

Overall, the system demonstrates a dynamically active state, likely undergoing significant structural transformation. Further spectroscopic analysis would be valuable in determining the individual redshifts and stellar populations of each component, as well as confirming the presence and composition of any tidal features.
