The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. There is a noticeable gradient in luminosity, with the core region exhibiting higher brightness compared to the outer regions. The galaxy exhibits a mild elongation, appearing somewhat cigar-shaped rather than perfectly circular. Color gradients are subtle, but a hint of bluer hues is discernible in the outer regions. It shows no clear evidence of spiral arms, bars, or significant tidal disturbances and appears relatively isolated.
