The galaxy presents as a relatively smooth, elliptical-like structure. Its central region exhibits a concentrated, bright luminosity, with the intensity diminishing outwards toward the edges. There is a suggestion of a subtle color gradient, transitioning from a yellow-orange hue in the nucleus to a slightly redder tinge in the outer regions of the halo, indicating an older stellar population present within. There are no spiral arms apparent, and it is generally spheroidal. The galaxy appears relatively undisturbed, with no signs of ongoing major mergers.
