The galaxy appears to be an interacting system. The primary galaxy exhibits a smooth, elliptical morphology with a concentrated central bulge. The color gradient indicates an older stellar population.

A smaller, bluer object is observed in close proximity. The blue color suggests ongoing star formation. This secondary object could be a dwarf galaxy in the process of merging with the primary, or a region of intense star formation triggered by gravitational interactions. There is evidence of tidal distortion in the primary galaxy, possibly from this interaction.

The overall structure suggests a galaxy that is relatively massive, with hints of low-level star formation occurring as a result of the interaction. Further spectroscopic analysis is required to determine the exact nature of the interaction and the star formation rate within both components.
