The galaxy appears as a centrally concentrated object with a relatively smooth morphology. The dominant light is yellowish-orange, suggesting an older stellar population. There is a hint of bluer light in the outer regions, possibly indicating some ongoing, though limited, star formation. The overall shape is close to circular, with no obvious spiral arms or bar structures. There are no indications of tidal tails or other major disturbances. The galaxy has a well-defined core, with a gradual decrease in brightness towards its outer edges. The galaxy is estimated to be of substantial mass, with only a modest star formation rate relative to its mass. Any merging is unlikely.
