The galaxy presents as a late-type spiral, observed nearly edge-on. A prominent central bulge dominates its morphology, appearing yellowish-orange, potentially indicative of an older stellar population. The galactic disk appears relatively thin and extended, exhibiting a subtle blueish-green hue, suggesting ongoing star formation within the disk. There is some indication of a boxy structure in the bulge. Overall, there do not appear to be any major disturbances or mergers in progress. The object is relatively smooth.
