The galaxy presents as a centrally concentrated object with a smooth overall morphology. Its color profile indicates a dominant population of older stars. The light distribution suggests an elliptical shape with a slight elongation. There is no evidence of spiral arms or a prominent disk. The object is relatively compact, with the light decreasing gradually from the center to its outer regions. There are no apparent signs of active star formation or significant dust lanes visible within the galaxy's body. The galaxy exhibits a fairly high Sersic index, indicating a steeper light profile characteristic of elliptical galaxies.
