The galaxy appears as a centrally concentrated, elliptical object with a high degree of smoothness. It exhibits a prolate morphology, appearing cigar-shaped rather than perfectly round. The light profile shows a gradual decrease in intensity from the core outwards, suggesting a relatively old stellar population. There is no apparent spiral arm structure or significant dust lane obscuration. Faint hints of a diffuse halo are discernible surrounding the galaxy, which does not show evidence of active merging or major tidal disturbances.
