The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal in shape. It exhibits a concentrated central bulge, with a gradual decrease in luminosity towards the outer regions, with a hint of a slightly elongated profile. The color profile suggests an older stellar population, with a yellow-red hue dominating the core, transitioning to a slightly greenish halo in the outer regions. There is little to no evidence of spiral arms or significant dust lanes. There are no signs of any major disturbances or mergers. Based on the smooth profile and color indices, this galaxy is likely a passively evolving system with suppressed recent star formation.
