This galaxy presents as a single, relatively smooth object with no obvious spiral arms or bar structure. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the edges. Its morphology is approximately elliptical, appearing mostly round. There are no visible signs of recent major mergers or significant tidal disturbances; however, there may be some minor disturbance. The galaxy's color suggests an older stellar population, potentially consisting of mostly Population II stars. Star formation activity is not apparently very high. The estimated size is relatively compact, meaning it is likely a small to medium sized galaxy.
