The galaxy presents as a spiral type, with a clearly defined disk structure. Spiral arms are discernible, though somewhat indistinct in the imagery. The winding of the spiral arms appears to be loosely distributed. The galaxy exhibits a substantial central bulge. There is no obvious bar structure visible. There are no clear signs of major mergers. The galaxy appears face-on relative to the observer's perspective. Color gradients suggest a population of younger, bluer stars within the spiral arms, in contrast to the central bulge, which displays a more yellow/red hue, indicative of an older stellar population.
