The galaxy exhibits a generally smooth morphology, with a slight elongation. It appears to have a concentrated central bulge that dominates the overall structure. The light distribution is relatively uniform, diminishing gradually from the center outwards. No distinct spiral arms or bar-like features are discernible. The overall color appears to be consistent with an older stellar population. There are no strong signs of recent major mergers or significant tidal disturbances in its immediate vicinity, although subtle disturbances are not entirely ruled out. The object is relatively compact in size.
