This galaxy presents an elliptical morphology, characterized by a smooth and centrally concentrated luminosity profile. The light distribution is noticeably more intense towards the galactic nucleus, exhibiting a gradual decrease in brightness as one moves outwards towards the periphery. There appears to be a slight elongation in the galaxy's shape, presenting a cigar like appearance. The galaxy has a slight blue tint in the outer edges which may indicate small amounts of star formation. No signs of spiral arms or a prominent disk structure are visible. There is no obvious major interaction or merging event currently in progress. The overall impression is of a mature, relatively undisturbed system.
