The galaxy presents as a slightly elongated, lenticular or early-type spiral, with a generally smooth, diffuse appearance. The central bulge is brighter and appears to be a yellow-white hue. The outer regions of the galaxy exhibit a bluer tinge, suggesting the presence of a younger stellar population. A faint disk-like structure may exist, though it is not sharply defined. There is a hint of some irregularity in the galaxy's shape, possibly indicative of minor tidal interactions or disturbances. The outer regions of the galaxy fade into the background, and there's a lack of strong spiral arm structure or prominent star-forming regions. Overall, it appears to be a fairly evolved galaxy, potentially undergoing a slow rate of star formation.
