The galaxy presents as a concentrated, elliptical morphology with a bright central bulge, suggesting a spheroidal stellar population. The color appears to be in the redder part of the spectrum, which could be indicative of an older stellar population with fewer hot, young stars and a higher proportion of red giant stars. There appears to be little evidence of spiral arms or significant dust lanes, though the resolution is limited. The light appears relatively uniform. Overall, the galaxy has a smooth and somewhat featureless appearance, suggestive of a relatively evolved and quiescent system.