The galaxy appears to be a somewhat smooth, centrally concentrated object, likely an early-type galaxy such as an elliptical or lenticular galaxy. There is a bright, yellowish central bulge, surrounded by a less luminous, more diffuse halo. The overall shape is close to round, though there is a slight elongation or asymmetry that could be indicative of tidal disturbances or an ongoing minor merger event. The color gradients suggest that the bulge is composed of an older stellar population, while the surrounding halo might contain relatively younger stars or dust. There is a hint of faint, wispy features in the outer regions, which could be tidal tails resulting from past interactions with other galaxies, although these features are not very prominent. There doesn't appear to be a disk component and it doesn't appear to be undergoing a major merger. The galaxy is relatively isolated in the image, suggesting that its evolution is less influenced by immediate galactic neighbors.
