The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. It appears approximately spheroidal in shape, tending towards "in between" elliptical classifications rather than perfectly circular. The light profile appears smoothly distributed without prominent spiral arms or a distinct disk. A slight elongation is observed. There is little evidence of significant morphological disturbances or ongoing merger activity, although subtle minor asymmetries cannot be entirely ruled out. Color gradients suggest that the core region exhibits a more yellow/red hue compared to the outer regions, which are less bright. The overall color of the galaxy suggests a population of older stars.
