This galaxy presents a disk-like morphology, observed at a significant angle from face-on, approaching edge-on. The central bulge exhibits a relatively smooth appearance and a concentrated luminosity profile. The disk component is more loosely defined, with hints of spiral arm structure, though these features are not sharply delineated. The overall color profile suggests active star formation, particularly in the disk regions, as evidenced by bluer hues in the outer reaches. There is some irregularity in the disk, which could be due to minor gravitational interactions. The disk appears to be more extended on one side as opposed to the other, adding to the overall asymmetry.
