The galaxy presents as a relatively smooth, elliptical-like structure, although not perfectly spherical. Its central region appears bright, suggesting a concentration of older stars. It is also possible the galaxy may contain an active galactic nucleus. A distinctive feature is an elongated structure projecting from the main body, appearing somewhat clumpy and potentially indicative of tidal debris. The galaxy exhibits a redder hue overall, implying an older stellar population and/or significant dust obscuration.
