The galaxy presents as a smooth, elliptical-like structure with a bright, concentrated core. It appears to be moderately massive and relatively quiescent in terms of star formation. There is little evidence of spiral arms or significant dust lanes; instead, it has a fairly uniform texture. Color gradients suggest a population of older stars dominating its composition, giving it a yellowish-white hue at its core. Its shape deviates slightly from being perfectly round, having an intermediate ellipticity, but it does not seem to display major distortions indicative of recent or ongoing merger activity, with the exception of a very slight tidal tail on the top right. The galaxy is relatively compact, with a half-light radius of less than 2 kpc.
