The galaxy presents as a generally smooth, elliptical-like structure with a centrally concentrated light profile. The core is notably brighter and exhibits a yellowish-white hue. The outer regions are less luminous, appearing more diffuse with a slight extension along its major axis, presenting a shape that's neither perfectly round nor highly elongated.

The color gradient suggests a population of older stars dominating the central region, while the outer regions may contain a younger, bluer stellar population, though this is less pronounced. There is no apparent evidence of a spiral structure, active star formation regions, or significant dust lanes. The overall morphology is consistent with an early-type galaxy, potentially an elliptical or lenticular galaxy seen at a slight angle. The galaxy exhibits a redder magnitude, indicating that the stellar population is not particularly young.
