The galaxy presents as a centrally concentrated object with a generally smooth morphology. The central region exhibits a high degree of luminosity, appearing almost uniformly bright. Fainter extensions can be observed extending outwards from the central region, with a relatively circular overall shape. The colors suggest a composition of older stellar populations, though some bluer regions may be present closer to the center, implying some ongoing star formation. There is no obvious sign of a spiral arm structure, or bar. The galaxy does not appear to be strongly interacting with any companion galaxies. Its overall structure suggests it could be an elliptical galaxy.
