The galaxy presents an elliptical morphology, appearing largely smooth with a centrally concentrated luminosity profile. The primary color of the galaxy is yellow-white, suggestive of an older stellar population dominated by lower-mass stars. A faint redder region is present, possibly indicating a small population of younger stars. The galaxy exhibits a slight disturbance, possibly due to a minor interaction or recent merger event. A faint, somewhat diffuse halo surrounds the central region, gradually fading into the background. The round shape of the galaxy indicates that the system has likely settled into a stable configuration, with minimal rotation or disruption of its overall structure.
