The galaxy presents as a pair of interacting objects. The larger component appears to be a relatively smooth, elliptical-like structure. It has a concentrated central bulge with a diffuse halo extending outwards. The color gradient suggests older stellar populations dominate, with a redder hue concentrated towards the core region, fading into yellowish tones in the outer halo.

The smaller interacting companion is visibly bluer in color, suggesting a younger stellar population and possibly ongoing star formation. It is less symmetrical and more compact compared to the larger galaxy. There are indications of tidal distortion in the larger galaxy, likely caused by the gravitational interaction with the smaller galaxy. These disturbances appear as faint extensions or asymmetries in the outer regions of the galaxy.
