The galaxy presents as a moderately bright object exhibiting a discernible morphology. The central region displays a concentrated, smooth bulge, suggestive of an older stellar population. Emanating from this central region is a faint, diffuse disk structure. There is some indication of very subtle spiral arm structure. The disk appears relatively undisturbed, but the color suggests some regions of current star formation. The overall shape of the galaxy is elliptical to lenticular, leaning towards a rounder morphology rather than a highly elongated form. There may be some minor gravitational interaction occurring. Overall, this galaxy appears to be in a relatively quiescent state.
