The galaxy exhibits a predominantly smooth morphology, with a centrally concentrated bulge. The overall shape approximates an elliptical form, appearing somewhat elongated rather than perfectly spherical. Faint, diffuse extensions of light suggest a possible disk component or tidal features, although these are not sharply defined. The central bulge presents a yellow-white color indicative of an older stellar population, whereas the outer regions show a slight bluer tint, possibly signaling ongoing or recent star formation within the galactic disk. There is no strong evidence of spiral arm structure, and the galaxy appears relatively undisturbed, lacking prominent signs of major mergers or significant tidal interactions.
