The galaxy presents as a relatively smooth, elliptical object with a noticeable central bulge. Its shape appears more elongated than perfectly spherical, exhibiting a cigar-like morphology. The core region displays a concentration of older stars, indicated by the redder hue. Fainter, greenish light appears at the outer edges of the galaxy. There is no strong evidence of spiral arms or a prominent disk structure. The overall appearance suggests a galaxy that has largely completed its major star formation phase, but the slight greenish hue around the outskirts implies some recent star formation activity, albeit at a low rate. There is no obvious evidence of ongoing major mergers or significant tidal disturbances, though minor asymmetries cannot be ruled out at this resolution.
