This galaxy presents an elliptical morphology, appearing somewhat elongated with a brighter, concentrated central bulge. The color profile suggests a population of older stars, exhibiting reddish-yellow hues in the core. Fainter, diffuse extensions are visible emanating from the main body, possibly indicating tidal debris or interactions with other galaxies. There is evidence of some disruption in the galaxy's structure, with the presence of asymmetrical features. Star formation rate appears to be relatively low in this galaxy.
