The galaxy presents as a moderately bright, elliptical structure. It exhibits a smooth, relatively featureless morphology with a noticeable central bulge that dominates the overall luminosity. The galaxy appears elongated, presenting an approximately cigar-shaped profile. There is a slight color gradient observed, with the central regions exhibiting a yellower hue suggestive of an older stellar population, transitioning to a bluer tint in the outer regions which is indicative of younger stars. The disk component, while present, seems subdued, with only subtle features and faint spiral arm structures. The lack of strong tidal features suggests the galaxy is not currently undergoing a major merger event, but some minor disturbances might be present. The overall appearance suggests a galaxy with a relatively high mass, potentially in the transition phase between a more actively star-forming system and a quiescent elliptical.
