The galaxy presents a predominantly smooth morphology. The primary body of the galaxy exhibits a somewhat rounded shape with a gradual transition to an intermediate ellipticity. There appears to be a notable disturbance present in the galaxy's structure, possibly suggestive of a minor interaction or tidal effect. The disturbance manifests as an arm-like asymmetry extending from the main body. The galaxy's color gradient indicates a concentration of older stellar populations in the central regions, with the outer regions showing evidence of ongoing or recent star formation activity. The relatively small size and high degree of smoothness suggest that this galaxy is a massive object with suppressed star formation.
