The galaxy presents as a relatively compact object. It exhibits a roughly elliptical morphology, though it is somewhat irregular in shape and the overall structure appears somewhat disturbed. The central region exhibits a bright, concentrated core. The color distribution suggests a dominant population of younger, bluer stars, concentrated in this central region. The outer regions appear fainter and redder. There is a clear change in color with radial distance. The smooth appearance suggests a lack of significant spiral arm structure or prominent dust lanes. Overall it appears to be intermediate between a spiral and elliptical galaxy based on the color distribution and morphology. There is no sign of it currently merging with another galaxy.