The galaxy presents as a somewhat elliptical, but mostly smooth, distribution of light. It has a bright, concentrated central bulge that gradually fades into a fainter, more diffuse halo. The light from the central region is relatively redder in color, transitioning to a slightly bluer hue in the outer regions. There is little to no apparent spiral arm structure or distinct features visible in the disk, suggesting a relatively evolved stellar population. The galaxy does not seem to be undergoing any major interactions or disturbances.
