The galaxy presents a largely smooth morphology, with minimal apparent spiral arm structure. The central bulge is prominent and exhibits a concentrated, yellowish hue, suggestive of an older stellar population. Fainter, bluer light surrounds the central bulge, indicating the presence of some ongoing star formation, albeit at a low rate. The galaxy appears generally elliptical, though it may also be described as disk-like, with little to no evidence of major disturbances or ongoing mergers. There is a subtle flattening, giving it a slightly elongated appearance. Overall, the galaxy presents as a relatively quiescent, evolved system.
