The galaxy presents a predominantly smooth, elliptical morphology. The light distribution is centrally concentrated, exhibiting a gradual decrease in intensity towards the outer regions. There is no distinct disk structure visible. The galaxy appears nearly round, with a subtle deviation towards a slightly elongated shape. No prominent spiral arms or bar features are discernible. There are no indications of ongoing major mergers or significant tidal disturbances. The overall color of the galaxy leans toward a redder hue, indicative of an older stellar population. The galaxy's estimated size is approximately 9 kiloparsecs in radius. The galaxy displays a low rate of star formation.
