This galaxy appears to be a relatively smooth, elliptical-type galaxy. Its overall shape is elongated, with a gradual decrease in brightness from the central region outwards. There is a bright central bulge and no easily discernable spiral arms or disk structure. It displays a generally blue hue, which might suggest some recent star formation activity, albeit likely at a low rate. The galaxy is not perfectly symmetrical, exhibiting some subtle irregularities in its outer regions, possibly indicating minor gravitational interactions or past mergers. The luminosity of the galaxy is relatively low, suggesting a smaller overall stellar mass compared to brighter galaxies.