The galaxy presents as a roughly elliptical object. The central region exhibits a bright, concentrated core with a slightly bluish hue. Moving outwards from the core, the light diffuses into a more extended, fainter halo. A slight elongation or disk-like structure may be present, but it is not clearly defined. The color appears to subtly redden in the outer regions, suggesting older stellar populations in the periphery. There does not appear to be any indication of major mergers or strong tidal disturbances in this image, and there is no distinct spiral arm structure. Overall, the galaxy appears relatively smooth, possibly suggesting a galaxy that is evolving passively.