The galaxy presents as a concentrated, largely featureless elliptical morphology with a prominent bulge. Its central region exhibits a yellowish hue, suggestive of an older stellar population. Moving outward, the galaxy smoothly transitions to fainter, greenish colors, likely due to a mix of older stars and possibly some younger populations or ongoing, though minimal, star formation. The overall shape appears somewhat elongated, falling between a round and cigar shape, suggesting a relatively undisturbed system. There are no visible signs of major mergers or significant tidal disturbances. The lack of prominent spiral arms or dust lanes supports the classification as an elliptical galaxy with a mostly smooth, evolved stellar distribution.
