The galaxy presents as a single, centrally concentrated object, characterized by a relatively smooth, featureless morphology in the observed wavelengths. The overall color appears to be yellowish-red, suggestive of a population of older stars. There is some elongation to the galaxy, with a hint of a possible tidal tail or plume in the lower portion, which could be indicative of a past or ongoing minor interaction. The nucleus of the galaxy appears to be relatively bright and concentrated, with an exponential light falloff toward the outer regions. There is no evidence of strong spiral arms or active star formation regions visible.
