The galaxy presents as a somewhat elongated, disk-like structure with a prominent central bulge. The bulge exhibits a yellow-orange hue, suggesting a population of older stars. Extending outwards from the bulge, the disk appears less defined, showing a slightly bluer color, potentially indicating regions of ongoing star formation, albeit seemingly at a modest rate. There is a subtle asymmetry evident in the disk's outer regions, hinting at possible past gravitational interactions or minor disturbances. The galaxy shows no signs of a clear spiral structure or active merging, and the overall form appears relatively smooth.
