The galaxy appears to be an elliptical, or lenticular, type. It exhibits a relatively smooth, symmetrical morphology, with no obvious spiral arms or distinct features. The central bulge appears bright and concentrated, with the light gradually fading towards the outer edges. There is a slight elongation, suggesting it is not perfectly spherical, perhaps more disk-like. The color gradient shows a yellowish hue in the center, potentially indicating an older stellar population with lower star formation activity, and a bluer tint towards the outer regions, which could be indicative of younger, hotter stars, or perhaps some ongoing low-level star formation. There are no obvious signs of tidal disturbances or interactions with other galaxies. Overall, it seems like a fairly evolved system.
