The galaxy presents as a largely smooth, elliptical-like structure, elongated along a primary axis. There is little discernible spiral arm structure. The light distribution suggests a centrally concentrated bulge, with a gradual decrease in surface brightness towards the outer regions. The color appears to be dominated by yellowish hues, suggestive of a stellar population that is relatively old and dominated by evolved stars. The morphological classification leans towards an elliptical, with a possibility of it being an edge-on lenticular galaxy, given the slightly flattened appearance. Evidences of tidal interactions or major mergers are subtle, however, minor disturbances cannot be ruled out given its faint irregular outer regions. The estimated size suggests a substantial galaxy. The rate of new stars being born appears quite low, in comparison to the total mass.
