The galaxy appears as a centrally concentrated object, exhibiting a smooth, relatively featureless morphology. The core region presents a bright, high-intensity luminosity, possibly indicating a substantial concentration of stars or an active galactic nucleus. The light distribution suggests a generally elliptical shape, with a subtle extension along its major axis. A diffuse, faint halo surrounds the central region, gradually fading into the background. The overall color profile seems consistent with an older stellar population, with a bias towards redder wavelengths. No prominent spiral arms or significant dust lanes are discernible. There are potentially minor disturbances and the galaxy may be in the process of merging.
