The galaxy presents as a somewhat elliptical or disk-like structure. It appears relatively smooth, with no readily apparent spiral arms or prominent features. The galaxy exhibits a slight elongation, appearing more oblate than perfectly spherical.

The color profile suggests a mix of stellar populations, with a concentration of yellowish light in the central region. Fainter, bluer light is visible extending outwards from the central bulge, hinting at regions of possible active star formation. There's also a hint of a diffuse, blue structure. 

The galaxy seems relatively isolated. There are no obvious signs of a major ongoing merger or strong tidal interactions with neighboring galaxies. Some faint, diffuse light surrounding the main body might indicate a stellar halo or evidence of minor disturbances. The galaxy has a notable presence, suggesting it is a galaxy of significant mass.
