The galaxy presents as an edge-on spiral or disk galaxy, with a prominent central bulge that appears relatively smooth and somewhat rounded. The bulge exhibits a concentrated, reddish color. The disk appears elongated and extends significantly beyond the bulge, displaying some evidence of structure though it is not clearly resolved. The outer regions of the disk show a bluer hue, possibly indicating the presence of younger stellar populations or ongoing star formation. There is a slight asymmetry visible in the disk's structure. The galaxy does not appear to be undergoing any major merging events, though minor disturbances cannot be ruled out based on the visual data alone. Overall, the galaxy appears well-formed and displays characteristics consistent with a massive, actively star-forming system at a considerable distance.
