The galaxy presents as a relatively smooth, disk-shaped structure. A bright, concentrated central bulge is visible, possibly indicating a supermassive black hole or a dense stellar population. The disk appears elongated, and slightly inclined. There are no apparent spiral arm structures. The light distribution suggests ongoing star formation, particularly in the disk region, which appears bluer compared to the central bulge. There's a suggestion of minor disturbances, possibly due to interactions with smaller galaxies. Overall, the galaxy seems to be a disk galaxy exhibiting characteristics of both early-type and late-type morphologies, but without strong, defined spiral arms.
