The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a centrally concentrated brightness profile, indicative of an older stellar population and minimal ongoing star formation. The color gradient shows a reddish hue in the central region, likely resulting from a high concentration of evolved stars. Moving outward from the core, the galaxy gradually fades into the background. The overall shape is roughly circular, with no obvious signs of spiral arms, bars, or significant morphological disturbances, suggesting it has likely undergone substantial morphological quiescence. There is some hint of a slightly extended halo or diffuse component around the main body of the galaxy.
