The galaxy presents as a moderately luminous, early-type system, exhibiting a largely smooth morphology. The light distribution is centrally concentrated, and there is little evidence of spiral arm structure or significant dust lanes. The object appears nearly circular, indicating a face-on or nearly face-on orientation with respect to our line of sight. 

There is a slight elongation, with a hint of tidal disturbances or a minor interaction with a smaller companion galaxy, which is nearby. Color gradients suggest the possibility of a faint, extended halo component, but it is very small.

The dominant color is yellow, with the secondary galaxy having a more green hue. The green hue suggests ongoing star formation regions, as suggested by the calculated star formation rate. Overall, the galaxy appears as a fairly massive system, based on its size and luminosity.
