The galaxy presents as a somewhat asymmetrical, diffuse structure. The central region exhibits a concentrated brightness, displaying a yellowish-white hue suggestive of an older stellar population. Extending outwards, fainter, somewhat disturbed features are observed, potentially indicative of ongoing or recent interactions with a neighboring galaxy. The overall color profile suggests a relatively evolved system with a mix of stellar ages present. Evidence of blue light from star formation may be present in some regions, but is relatively muted compared to other wavelengths. The galaxy is not distinctly spiral or elliptical but displays features of both morphological types.
