This galaxy appears to be a relatively smooth, elliptical galaxy with a somewhat spherical morphology. The central region exhibits a higher surface brightness, indicative of a concentrated stellar population. The galaxy displays a radial color gradient, transitioning from a yellowish-white core to bluer outer regions, possibly suggesting a more metal-poor stellar population or ongoing star formation activity in the periphery. There is no strong indication of a prominent disk structure or spiral arms. Faint, diffuse features might be present, though they could also be artifacts of image processing or blending with background light. The overall impression is that of a relatively evolved galaxy, potentially undergoing minor interactions or exhibiting residual star formation. There is very little dust apparent. There are no disturbances or mergers detected in this image.
