The galaxy presents as a relatively smooth and concentrated object. Its shape is generally elliptical, though not perfectly round, appearing slightly elongated. There is no discernible disk structure or spiral arm morphology; instead, a smooth and featureless distribution of light is observed across the galaxy's body. There is a slight suggestion of a brighter central region, which may correspond to a galactic bulge. No signs of ongoing major mergers or significant tidal disturbances are apparent. The galaxy displays a color profile suggesting a population of older stars and, based on its colors, it appears to be undergoing low levels of star formation.
