The galaxy presents a generally smooth, elliptical morphology, with a dominant central bulge that is very bright and concentrated. The light intensity decreases gradually from the center outward. There is some indication of a flattened disk, but the bulge dominates the overall shape. There are some faint asymmetric extensions or tidal features on one side. Its overall color appears relatively uniform, suggesting a lack of significant dust lanes or distinct star-forming regions. No spiral arm structure is visible, supporting the classification as an elliptical or lenticular galaxy. The galaxy appears relatively isolated, with no obvious signs of ongoing major merger activity, although there is potentially some minor disturbance of the galaxy from an unseen companion, if the faint asymmetric extensions are indeed real.
