The galaxy presents as a centrally concentrated system with a primarily smooth morphology. The core exhibits a bright, yellowish-white hue, suggestive of an older stellar population. The galaxy exhibits an elliptical shape with a slight elongation. A faint, small region of blue-green coloration is visible along the galaxy's periphery, potentially indicating a region of more recent star formation activity. There are no obvious signs of major mergers or significant tidal disturbances, however there is a slight asymmetry in the color distribution.
