This galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits a high concentration of light, appearing bright and somewhat reddish in color, possibly indicating an older stellar population. Moving outward from the core, the luminosity gradually decreases with a more diffuse, bluish halo surrounding the central bulge. There is a slight deviation from perfect roundness, leaning more towards an in-between elliptical shape. Overall, the galaxy lacks any obvious signs of recent major mergers or significant disturbances, and shows no clear spiral arm structure.
