The galaxy presents as a single, mostly smooth, centralized object. Its light is concentrated, showing a structure without defined spiral arms or a prominent bar. The central region appears brighter and somewhat diffuse, potentially indicating a high concentration of stars or an active galactic nucleus. There is a very slight elongation, as the galaxy is not perfectly circular, but is close to round. The overall color is slightly yellowish, indicating a population of older stars. There is no apparent evidence of major tidal distortions or ongoing mergers, although there is very faint indication of some possible minor disturbance.
