The observed galaxy presents as a disk galaxy, seen nearly edge-on from our vantage point. A prominent, relatively bright central bulge dominates the structure, exhibiting a smooth, round appearance with a concentration of light in its core. The galaxy shows no signs of major interaction or disturbance but possibly some minor disturbance. The disk appears thin and elongated and it may contain some dust features that are difficult to make out. Overall, the galaxy exhibits a structure consistent with an actively star-forming disk galaxy.
