The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in surface brightness moving outward from the core. The color is generally consistent across the galaxy, appearing slightly redder than the surrounding field. There is little evidence of spiral arms or significant dust lanes. Minor asymmetries may be present upon closer inspection, potentially indicative of minor gravitational interactions or internal dynamical processes. The overall impression is of a relatively quiescent system, likely dominated by an older stellar population.