The galaxy presents as a spiral galaxy with a prominent disk structure. The spiral arms are clearly visible, showing a distinct pattern that winds moderately tightly around the central bulge. There is a high probability that this galaxy has spiral arms, there is a visible bar structure that bisects the central bulge, though it could be categorized as weak. The bulge itself appears to be moderate in size relative to the overall disk, and the galaxy is not seen edge-on. The galaxy exhibits colors that are indicative of ongoing star formation, with regions of bluer light interspersed within the spiral arms, as well as hints of possible disturbances in it's spiral arms.
