This galaxy presents as a relatively small, disk-shaped structure. The central region exhibits a high degree of surface brightness, appearing almost point-like, which could be indicative of an active galactic nucleus or a dense stellar population in the bulge. Emanating from the bright center, a flattened disk is visible. The disk displays a mottled texture, possibly indicating the presence of star-forming regions or dust lanes. A slight asymmetry is discernible in the outer regions of the disk, with one side appearing slightly more extended or disturbed than the other, possibly suggesting a minor interaction or gravitational disturbance. The color gradient across the galaxy transitions from a bluer hue at the center to a greener hue towards the outer edges of the disk, possibly indicating differing stellar populations or dust composition. Overall, this galaxy appears to be a relatively unremarkable, albeit slightly perturbed, disk galaxy.
