The galaxy presents a generally smooth, elliptical morphology, exhibiting a concentrated central bulge. The light distribution appears centrally dominant, with a gradual fall-off towards the outer regions. The color profile suggests a population of older stars, indicated by the redder hue in the central regions, transitioning to slightly bluer tones at the galaxy's periphery. There are no prominent spiral arms or dust lanes visible. No strong tidal features, or indications of major mergers, are apparent in the immediate vicinity of the galaxy.
