The galaxy exhibits a generally elliptical morphology, appearing to have a relatively smooth structure. The central region shows a high surface brightness, indicative of a concentrated stellar population or active galactic nucleus. Surrounding the bright center, there's an extended disk or halo of lower surface brightness material. Some subtle features, such as faint wisps or asymmetries, suggest possible minor disturbances in the gravitational potential, perhaps due to recent or ongoing minor mergers or tidal interactions. Overall, the galaxy seems to have properties consistent with an early-type spiral galaxy.
