The galaxy presents a generally smooth, elliptical morphology. The central bulge appears prominent and relatively bright with a yellow-orange hue, suggesting a population of older stars. There is little evidence of spiral arms or significant dust lanes. The galaxy's overall shape is slightly elongated, appearing somewhere between round and cigar-shaped. There are no obvious signs of ongoing major mergers or significant tidal disturbances, though there are subtle asymmetries in the outer regions that might suggest minor gravitational interactions or past disturbances. Based on the color profile, there is a faint hint of bluer light in the outer regions, which could indicate some low-level recent star formation.
