The galaxy presents a largely smooth morphology, exhibiting characteristics consistent with an elliptical galaxy. The light distribution appears centrally concentrated with a gradual decrease in intensity towards the outer regions. There is a slight elongation, but the overall shape is mostly round. Color gradients are subtle, with a slightly yellower core transitioning to redder hues in the outer regions, possibly indicating an older stellar population throughout the galaxy. No distinct spiral arms, dust lanes, or other features typically associated with disk galaxies are readily apparent in this image. There appears to be no significant signs of ongoing merger activity or major tidal disturbances.
