The galaxy presents as a single, relatively smooth object, exhibiting a concentrated central bulge that radiates prominently. This luminous core fades gradually into the outer regions of the galaxy, indicating a lack of significant spiral arm structure. The object is quite round in appearance. The overall color profile suggests a population of older stars, as evidenced by the redder hue, but there may be some recent star formation as the center has a slightly more green/blue tint. No major disturbances or mergers are readily apparent.
