The galaxy presents an overall smooth morphology, with a somewhat elongated shape suggesting it is not perfectly spherical. Its light distribution appears centrally concentrated, diminishing in intensity outwards. There is a subtle color gradient, with the central region appearing more yellow, potentially indicative of an older stellar population. The outer regions exhibit a bluer tinge, hinting at the presence of younger stars or ongoing star formation. Weak asymmetries are visible, perhaps due to minor tidal interactions or internal disturbances, but no distinct spiral arm structures or prominent features are readily apparent.
