The galaxy presents a generally elliptical morphology. It exhibits a smooth, diffuse light distribution without any discernible spiral arm structures or prominent dust lanes within this image. The core is a bright region that gradually fades outward into the galaxy's halo. There is a slight bluing of the light in the outer regions, with the core appearing more yellow. This suggests a possible difference in stellar populations, with younger, bluer stars residing towards the outskirts, and older, redder stars concentrated towards the center. The shape is somewhat elongated, indicating it is not perfectly spherical. There is no apparent sign of interactions with other galaxies.