The galaxy presents a generally smooth and rounded morphology. It appears somewhat elliptical in shape, though not highly elongated. The light distribution is concentrated towards the center, indicating a prominent bulge. There is a subtle indication of a possible disk component, but this is not very distinct in the image.

Color gradients suggest older stellar populations dominate this galaxy. There might be minor disturbances but it looks relatively isolated, without any obvious signs of recent or ongoing major mergers or strong tidal interactions.
