The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a prominent bulge and a disk-like structure. The bulge is centrally located and dominates the galaxy's overall luminosity, appearing smooth and featureless with a yellowish-white hue, suggestive of an older stellar population.

Surrounding the bulge is a fainter, flattened disk. The disk shows subtle hints of spiral arm structure, although these are not sharply defined. The outer regions of the disk fade gradually into the background sky. Patches of slightly bluer light are observed within the disk, possibly indicating regions of recent or ongoing star formation. The disk also displays some dust lanes, visible as subtle dark bands silhouetted against the background starlight.

The galaxy's overall morphology suggests it is a relatively massive system. The smoothness and roundness of the bulge, combined with the subtle disk features, point towards a galaxy that is transitioning from a more active, star-forming state to a more quiescent one. It is not currently undergoing any major merger activity, although there may be subtle signs of past interactions or minor disturbances in its outer regions.
