The galaxy presents a generally smooth and elliptical morphology. It exhibits a concentrated central bulge that appears yellowish in color, suggesting a population of older stars. The outer regions are fainter and appear to transition towards a redder hue. There is little evidence of spiral arm structure or significant dust lanes. The overall appearance suggests a relatively evolved system with a low star formation rate. There are no obvious signs of ongoing mergers or tidal disturbances, with a very slight asymmetric halo on one side. The galaxy's shape is somewhere in-between elliptical and a flattened disk.
