The galaxy presents as a relatively smooth and elongated structure. It appears to be a disk galaxy observed at a significant angle. The central bulge exhibits a yellowish hue, potentially indicative of an older stellar population and/or dust obscuration. The disk, while not clearly resolved into spiral arms, shows a subtle color gradient, fading from yellowish-white near the bulge to a bluer tint at the edges, possibly suggesting ongoing star formation in the outer regions. The overall morphology indicates a low star formation rate and a substantial stellar mass. There are some disturbances in the smoothness of the galaxy, potentially caused by minor mergers. The galaxy appears to be significantly cigar shaped.
