The galaxy presents as a disk galaxy, likely viewed edge-on or close to edge-on, as indicated by its elongated morphology. A distinct bulge is not readily apparent, suggesting it may be relatively small or obscured by dust. The central region exhibits a bluer hue compared to the outer regions of the disk, possibly indicating ongoing star formation activity, although it is not very pronounced. The dust lane appears to be complex and relatively undisturbed suggesting that the morphology is likely maintained, and the star formation rate is moderately suppressed. It may have experienced a minor merger or gravitational interaction in the past, but it does not appear to be currently merging. There is a plume-like structure above the galaxy, which could indicate some kind of event has disturbed the structure of the galaxy.