The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears to be elliptical, elongated along one axis. There is a bright central bulge region, surrounded by a fainter, more diffuse halo. The color profile suggests a predominantly older stellar population, with a slight bluer component towards the outer regions; though this is minimal. There is no clear evidence of spiral arm structure or significant dust lanes, and the morphology appears largely undisturbed. The galaxy shows no obvious signs of ongoing major merging activity, and no severe gravitational disturbances.
