The galaxy presents a primarily smooth appearance with a central bulge that exhibits a warmer, redder hue, suggesting a population of older stars. A fainter, bluer disk surrounds the bulge. The disk itself does not appear to have any strong spiral arm structure or clumpy star forming regions, rather a diffuse blueness. The overall shape is somewhere between round and elongated, tending more towards elliptical than a perfect sphere, possibly classified as an S0 or early-type spiral. There is a subtle suggestion of a tidal feature or minor distortion in the outer regions of the disk, indicating a possible recent or ongoing interaction with a smaller companion galaxy. The estimated size and shape of the galaxy is relatively compact.
