The galaxy presents as a centrally concentrated, elliptical morphology with a smooth light distribution. There is little evidence of distinct spiral arms or prominent star-forming regions. The core appears relatively bright, transitioning into a more diffuse halo. The overall color suggests a population of older stars, with a notable lack of blue indicative of younger stellar populations. The galaxy exhibits a slight elongation. There is a possible hint of minor asymmetry, though it appears mostly relaxed in its morphology. The galaxy appears to be relatively isolated with no signs of major interactions with neighboring galaxies.
