The galaxy exhibits a generally smooth morphology, appearing elliptical in shape. The central region displays a concentrated, bright core with a yellow-white hue, potentially indicating an older stellar population. Moving outward from the core, the light becomes less concentrated and shifts slightly towards redder colors, likely from older stars or dust. There may be faint suggestions of a disk-like structure, but its presence is not clearly defined. The overall appearance suggests a galaxy that has largely settled into a relatively quiescent state. There is no obvious visual evidence of on-going major mergers or tidal disruptions. Close inspection reveals no obvious spiral arm structure, and the smoothness and shape of the object suggest it is most likely an elliptical galaxy at a moderate distance.
