The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a smooth, fairly symmetrical morphology. There is no discernible spiral arm structure or bar. The core region appears to be brighter and more yellow in color, suggesting an older stellar population. The outer regions have a more diffuse appearance, with a bluer hue, perhaps indicating more recent star formation activity. There appears to be a slight asymmetry or minor disturbance on one side, although there is no obvious sign of an ongoing major merger event. The overall structure appears relatively undisturbed, with no distinct tidal tails or bridges.
