This galaxy appears to be an elliptical type, exhibiting a generally smooth and diffuse light distribution. The central region displays a slightly higher concentration of luminosity. The overall shape is moderately elliptical, elongated along a major axis. There is a suggestion of tidal features, possibly indicative of a recent or ongoing interaction or merger event. A subtle disturbance or asymmetry can be seen, particularly extending outward from one side, lending support to the interaction hypothesis. The galaxy possesses a population of older stars, indicated by the color. Star formation is likely minimal.