The galaxy presents a generally smooth and concentrated appearance, indicative of an elliptical morphology, though a slight elongation is observed along its major axis. Its color profile suggests a population dominated by older stars, emitting a yellowish to reddish hue. There is no obvious structure like spiral arms or dust lanes. Faint, diffuse extensions are present around the central region, perhaps indicative of a halo component. The overall light distribution is relatively uniform. Possible minor gravitational disturbance may be present, though it does not appear to be merging with another galaxy. 
