The galaxy presents a generally smooth and centrally concentrated morphology. It exhibits a slightly elliptical shape, appearing more "in-between" round and elongated. The galaxy lacks any apparent spiral arm structure or strong features indicative of ongoing major mergers. There is a slight color gradient, transitioning from a bluer core region to redder outer regions. This suggests a change in stellar population, with the core possibly containing younger, hotter stars and the outskirts containing older, cooler stars. The galaxy's size is relatively modest. There are no apparent signs of dust lanes or significant tidal disturbances. Subtle irregular features might suggest minor past interactions, but it is predominantly a well-defined system.
