The galaxy presents a generally smooth, elliptical morphology. It exhibits a dominant, centrally concentrated luminosity profile, appearing quite round in shape. The galaxy displays a yellowish-orange hue, suggestive of a relatively older stellar population with less ongoing star formation. A faint, diffuse halo may be present, extending slightly beyond the brighter central region, although the signal-to-noise ratio makes it difficult to discern clear structural details. There is evidence of a possible minor disturbance or interaction; a small amount of asymmetry is present, perhaps caused by a very minor tidal interaction with another galaxy. The system does not show any signs of major merging activity or significant tidal tails.
