The galaxy presents as a relatively flat, disk-shaped structure, with a prominent central bulge that transitions smoothly into the disk. There is a slight asymmetry in the morphology of the disk. The color gradient across the galaxy suggests a compositional variation. One side exhibits a bluer hue, potentially indicative of ongoing star formation, while the other side displays slightly redder tones. The galaxy shows evidence of potential disturbance, with a slight warp, or perhaps a tidal tail, on one side. There also appears to be a faint feature near the center of the galaxy, possibly indicative of a recent merger or interaction. Overall, it appears to be a spiral-type galaxy, with low contrast between the bulge and disk regions, and a general lack of spiral arm structure.
