The galaxy presents as a generally smooth, ellipsoidal object, with a noticeable concentration of light towards the center. There appear to be two distinct components, possibly indicative of a merger. The northern component exhibits a yellower hue compared to the southern component which appears bluer. The light distribution suggests that the galaxy is relatively compact, and there are no obvious spiral arm features or significant dust lanes visible. There is a slight asymmetry in the light distribution, hinting at potential tidal interactions or ongoing merger activity.
