The galaxy presents as a relatively smooth and flattened structure, appearing primarily elliptical. Its central region exhibits a higher concentration of light, with a color index suggesting an older stellar population, likely dominated by redder, evolved stars. This central bulge is elongated along the major axis of the galaxy. 

Surrounding the central bulge is a less concentrated, bluer disk. The disk appears to be comprised of more active star formation regions. The color suggests the presence of a younger, hotter stellar population.

The image shows evidence of a possible tidal interaction or minor disturbance in the form of an apparent plume of material extending outwards. There also appears to be a second smaller galaxy in the midst of merging with the larger galaxy.
