This galaxy presents as a relatively smooth, elliptical morphology with a dominant, centrally concentrated bulge. The overall shape is largely rounded. There are regions of redder emission near the core, indicative of an older stellar population or dust obscuration. However, there is also a region of bluer emission at the galactic periphery, suggestive of younger stars. Based on its estimated size, it appears to be a moderately sized galaxy. Despite the general smoothness, there are subtle irregularities in the light distribution, hinting at a possible minor interaction or disturbance.
