The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile is dominated by yellow and red hues in the central region, suggestive of an older stellar population and potentially lower levels of ongoing star formation. There's a subtle transition to bluish colors towards the outer regions, hinting at the presence of younger, hotter stars, though not in a pronounced spiral arm structure. The overall morphology appears undisturbed, showing no significant signs of tidal interactions or major mergers. There is an slight asymmetry in the light distribution, but it does not appear to indicate a major disturbance. It appears to be quite round in shape, rather than elongated.
