The galaxy presents as a relatively face-on lenticular or early-type spiral. It exhibits a smooth, centrally concentrated bulge that is distinctly yellow-orange in color, indicative of an older stellar population. There is evidence of a flattened disk component surrounding the bulge, but spiral arm structure is not immediately apparent. The disk exhibits a bluer color than the central bulge, suggesting the presence of younger, hotter stars, although the star formation rate appears low. The overall morphology suggests a galaxy that is transitioning, or has already transitioned, from active star formation to a more quiescent state. The shape of the galaxy is somewhere between round and cigar shaped. There appear to be no signs of any major ongoing mergers, or major disturbances, although there might be some sort of minor disturbances or tidal debris, but not enough to see clearly.
