The galaxy presents a largely smooth, elliptical morphology. The light distribution suggests a high degree of radial symmetry, with a concentration of luminosity towards the center. It exhibits a subtle color gradient, transitioning from a more yellow-hued central region to a slightly bluer outer halo. There is little evidence of distinct spiral arms, prominent dust lanes, or significant star-forming regions, which is consistent with an older stellar population. A very slight asymmetry in the outer halo might suggest a possible minor interaction or past merger event.
