The galaxy presents as an elongated, cigar-shaped object with a smooth, concentrated central bulge. The color profile suggests a dominance of older stellar populations, indicated by the reddish-yellow hue. There are subtle hints of a disk-like structure extending from the central bulge, though its features are not sharply defined. There's no evidence of significant dust lanes or prominent spiral arm structures. Overall, the galaxy appears relatively undisturbed, showing no signs of a recent major merger event, though subtle signs of minor disturbances cannot be ruled out.
