The galaxy presents a roughly elliptical morphology. A bright, concentrated central bulge is apparent, emitting strongly in the redder wavelengths. Fainter spiral arms extend outwards from the bulge region, showing a hint of bluer colors, suggesting the presence of some recent star formation in these regions, although this is minimal. The galaxy has a fairly smooth overall appearance, with no obvious signs of major mergers or strong tidal disturbances and the disk is being viewed at an angle. There is a suggestion of a bar in the center of the galaxy.
