The galaxy presents as a relatively smooth, elliptical-like structure. Its morphology is dominated by a centrally concentrated bulge, which exhibits a yellowish-white color. This core region appears quite bright and dense, indicative of a significant population of older stars. Extending outward from the central bulge is a fainter, diffuse halo. There's little to no evidence of spiral arm structure. The galaxy appears isolated. The overall color profile suggests an evolved stellar population, possibly indicating a relatively low rate of ongoing star formation. Any star formation would appear to be limited in its extent and intensity. There is no evidence of significant dust lanes or other features indicative of active star formation or recent merger events. The galaxy is most likely a massive, passive galaxy.
