The galaxy presents as a centrally concentrated, elliptical system. It exhibits a smooth, diffuse morphology, lacking prominent spiral arms or distinct features. The central region is notably brighter, suggesting a concentrated stellar population or active galactic nucleus. The galaxy appears flattened, but not highly elongated. There's a gentle gradient in color, with a slightly bluer outer halo, indicating some star formation. There are no obvious signs of ongoing major mergers or significant tidal disturbances, but some minor distortions may be present. The galaxy is estimated to be relatively massive, based on its overall luminosity and size. The star formation rate is low but non-zero, suggesting a transition stage between a strongly star-forming spiral and a quiescent elliptical galaxy.