The galaxy presents an overall elliptical morphology, appearing rather smooth in texture. Its core region exhibits a bright, concentrated luminosity, transitioning to a less intense, extended halo. Color gradients are subtle but visible; the central region leans toward warmer, yellower hues, possibly indicating an older stellar population or dust obscuration. The outer regions present a cooler, bluer tone, indicative of the potential presence of younger, hotter stars, or ongoing, but small, star formation activity. There is a hint of a slight spiral structure; some regions are somewhat disturbed or clumpy. Overall, the galaxy seems to be relatively isolated with no obvious signs of ongoing major interactions or mergers. Its axial ratio suggests an oblate spheroid shape.