The galaxy presents a generally smooth, elliptical morphology. Its color appears largely homogenous, exhibiting a yellowish-white hue, suggesting a population dominated by older stars. There are no readily apparent spiral arm structures or significant dust lanes. The light profile appears relatively concentrated towards the center, indicative of a bulge-dominated system. No obvious tidal features or strong gravitational distortions are observed, suggesting it is not currently undergoing a major merger event. The overall structure suggests a relatively evolved galaxy with a subdued star formation rate. There appears to be a slight asymmetry in the isophotes, indicating a possible minor interaction or internal disturbance.
