The galaxy presents as a relatively smooth, lenticular-like structure with a slight elongation. There is an appearance of a dust lane and or other type of absorption of light on the left side of the galaxy, with bluer light. The overall shape indicates a possible transitionary phase, from a more active spiral to a quiescent elliptical galaxy. Some sort of disturbance may be present. The galaxy shows a smooth profile, and a centrally concentrated bulge. The presence of a faint disk cannot be ruled out. The colour gradient suggests the presence of an older stellar population, especially in the central bulge, however the bluer light on the left side could indicate a younger population. The overall morphology indicates a system that has experienced some evolutionary changes, hinting at a possible interaction or past merger event. Star formation may be low, although the bluer light on one side may be related to a modest level of on-going activity.