The galaxy presents as a centrally condensed, roughly elliptical structure. A bright, yellowish core dominates the central region, suggesting a significant concentration of older stars. Moving outward from the core, the light transitions to a bluer hue, forming an extended halo around the core region. The overall morphology suggests a galaxy that is primarily smooth and relatively undisturbed. There is a hint of subtle structure or faint arm-like features in the disk region, but they are not sharply defined. The galaxy appears to be relatively isolated. There is a possible tidal feature or streamer of material extending from one side of the disk.
