The galaxy presents as a relatively compact, elliptical-like structure. It exhibits a smooth luminosity profile, with a noticeable central concentration. While appearing mostly smooth, there is a hint of a disk-like component or faint spiral arms. The color distribution shows a redder hue in the central region, potentially indicative of an older stellar population, gradually transitioning to bluer colors in the outer regions, possibly indicating the presence of younger stars. A minor disturbance is observed in its morphology, indicating a possible past or ongoing interaction. The overall shape is mostly round.
