This galaxy appears to be a spiral galaxy, observed at an oblique angle, but not quite edge-on. There is a central bulge that appears to be bright and roughly spheroidal, with a yellow-orange color profile, suggesting an older stellar population. The disk of the galaxy shows some structure that indicates the possibility of spiral arms, with pockets of bluish coloration mixed with areas of reddish-orange, implying variations in star formation activity and dust content across the disk. The blue areas indicate a small amount of younger, hotter stars are present. It is difficult to clearly resolve distinct spiral arm structures. There's a slight asymmetry in the outer regions of the galaxy, with the disk appearing slightly more extended on one side. There are no obvious signs of recent major merging events, though a slight disturbance to the symmetry of the disk exists.
