The galaxy presents a generally smooth, elliptical morphology. The central region appears as a bright, unresolved core, suggesting a high concentration of stars. Progressing outward from the core, the luminosity decreases gradually. There's little evidence of distinct spiral arms or significant dust lanes. The overall color is relatively uniform, trending towards bluer hues in the outer regions. This could indicate the presence of a younger stellar population or ongoing star formation, however, the smooth profile of the galaxy, and lack of features like defined spiral arms or significant irregular structure suggests a largely quiescent object. A small amount of disturbed morphology may suggest that a merger or tidal interaction could be ongoing.
