The galaxy presents as a face-on or nearly face-on spiral galaxy, with a central bulge and a faint, blue-tinged disk. There is a prominent central concentration of light, suggesting a bulge of older stars. The disk exhibits a mottled texture, potentially indicating regions of ongoing or recent star formation. There is a subtle asymmetry in the disk's distribution of light, with one side appearing slightly more extended or disturbed than the other. This could be indicative of a minor interaction with another galaxy or an internal process disrupting the disk structure. Overall, the galaxy appears relatively normal, showing characteristics of both smooth, well-defined spiral structure and hints of possible interaction or disturbance. The galaxy has a moderate to high redshift, placing it at a considerable cosmological distance.