The galaxy presents as a fairly smooth, elliptical-like structure. It exhibits a concentrated central bulge with a diffuse, extended halo of light. The color profile suggests a population of older stars, as evidenced by the redder hue. There is a notable lack of defined spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, without strong indications of recent major mergers or interactions. The overall shape is somewhat round, with a hint of elongation. There is also a point of light to the right side of the galaxy, the nature of which is unclear.
