The galaxy presents a smooth, elongated morphology, suggestive of an elliptical type. The light distribution exhibits a central concentration with a gradual decrease in intensity towards the outer regions. A slight color gradient is observed, with a yellower hue dominating the central region, possibly indicating an older stellar population. The outer regions appear somewhat bluer, which might be due to the presence of younger stars. There is no visible evidence of spiral arms or a prominent disk structure. The overall appearance indicates a relatively quiescent galaxy with minimal ongoing star formation. The shape appears more cigar-like than round. There do not appear to be any obvious signs of merging activity or major disturbances.
