The galaxy presents as a fairly smooth, elliptical structure with a bright, concentrated central bulge. The overall shape tends toward being somewhat in between round and elliptical, but is mostly in between, lacking a highly defined disk or spiral arms. There is faint evidence of minor disturbances, but these are not overtly dominant features, suggesting no recent major merger event. The galaxy displays a subtle color gradient, with the central region appearing slightly bluer than the outer regions, indicating the potential for some ongoing star formation activity, albeit at a low rate. The galaxy's apparent size is small, hinting at a relatively low mass.
