The galaxy presents as a relatively compact and bright object. It exhibits a general smoothness in its overall appearance, with no immediately obvious spiral arm structures or prominent dust lanes. The morphology appears largely elliptical or lenticular, though some slight elongation may be present.

The light distribution is concentrated, with a brighter core region that fades gradually towards the outer edges. A faint, extended halo may be present but difficult to observe due to image limitations. Color gradients seem subtle, suggesting a relatively homogenous stellar population, with older stars. There may be slight evidence of some ongoing star formation, though not at a particularly intense rate. There may also be the possibility of minor interactions based on its profile.
