The galaxy presents as an elongated structure, likely a disk galaxy viewed at an oblique angle. The central bulge appears prominent and exhibits a yellowish hue, indicative of an older stellar population. Extending outwards from the central bulge, the disk displays a mottled texture, possibly revealing the presence of spiral arms, though these are not sharply defined. The outer regions of the disk show a bluer coloration, suggesting the presence of younger, hotter stars within the spiral arms. The dust lanes may be slightly obscuring areas. The overall morphology indicates a galaxy undergoing active star formation, particularly in the outer regions of the disk, with a more quiescent, evolved stellar population dominating the central bulge. There seems to be slight evidence of some tidal disturbance in the form of a faint stream of material extending from one edge of the galaxy.
