The galaxy presents as a centrally concentrated, elliptical-like structure. A smooth, diffuse light profile characterizes its morphology. The core region exhibits a distinct yellowish hue, possibly indicating an older stellar population or a significant dust component. There is no apparent disk structure or spiral arms, and there is no noticeable evidence of current merging activity or major tidal disturbances. The outer regions of the galaxy are less distinct and appear to fade into the background sky with a reddish tint. Overall, the galaxy exhibits a smooth, relatively undisturbed appearance suggesting a fairly evolved system.
