The galaxy presents as a somewhat elongated, likely disk-shaped structure, viewed at a significant angle. The central bulge appears prominent, exhibiting a reddish-orange hue, possibly indicating an older stellar population. The overall color of the galaxy shifts to a slightly bluer tone in the outer regions of the disk, hinting at younger, hotter stars and ongoing star formation within the spiral arms, if any exist. The morphology suggests it is an undisturbed galaxy. It appears relatively smooth, with no obvious signs of interaction or merging events. The shape is cigar-shaped with the longer axis more than twice the length of the shorter axis. There is a clear separation between the bulge and the outer structure.
