The galaxy presents as a centrally concentrated, elliptical morphology, with a smooth light distribution. The core region exhibits a pronounced yellowish-orange hue, which subtly fades towards the outer regions. The observed color suggests a stellar population dominated by older, redder stars. No distinct spiral arm structures or dust lanes are discernible. The overall appearance suggests a relatively evolved system. There is the suggestion of minor disturbances around the edges, indicating possible gravitational interactions with smaller galaxies.
