The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. A discernible nucleus, characterized by a yellow hue, is centrally located and dominates the galaxy's light profile. Moving outward from the core, the color shifts subtly to redder tones suggesting a stellar population comprised of older, cooler stars. There is little evidence of spiral arms, dust lanes, or active star-forming regions based on the color distribution. The galaxy lacks features associated with recent or ongoing merger activity, retaining a largely undisturbed, spheroidal appearance. Overall, it suggests an evolved system dominated by an older stellar population.
