The galaxy presents as a flattened elliptical or lenticular form. Its central region exhibits a high surface brightness, appearing almost spheroidal with a concentrated, bright core. Moving outward from the core, the light gradually diminishes into a diffuse halo. The light from the core is predominantly bluish-white, suggesting the presence of relatively young stars or a hot, ionized gas. Surrounding the central region, a faint, extended disk is present, its color trending toward redder hues, potentially indicating a population of older stars. There are subtle indications of mild disturbances or asymmetries in the outer regions of the galaxy. It exhibits a degree of elongation, with the major axis significantly larger than the minor axis. Overall, the galaxy's appearance suggests it is relatively massive. Star formation may be occurring at a low rate.
