The galaxy presents a generally smooth, elliptical morphology. Its light is concentrated towards the center, exhibiting a bright, well-defined core. The isophotes appear roughly circular, transitioning to a slightly elongated shape along its radial axis. There is a lack of distinct spiral arms or prominent dust lanes. The overall color profile suggests a population dominated by older stars, emitting strongly in redder wavelengths, with a moderate signal in green and somewhat lower signal in blue wavelengths. There seems to be a possible companion galaxy to the southeast. Based on its appearance, this is likely a relatively massive galaxy that is not currently experiencing a high rate of star formation. There do not appear to be any major disturbances that might suggest a recent major merger event, but a minor interaction is possible.