The galaxy presents as a lenticular or possibly an edge-on spiral galaxy. Its shape is elongated, with a pronounced central bulge that appears yellowish-white, indicative of an older stellar population. A fainter, bluish component is visible as a disk-like structure. There appears to be a dwarf galaxy or group of stars in the distance on the left side of the frame. The morphology suggests a system undergoing or that has recently undergone an interaction that may be disturbing its structure. This galaxy is a mid-mass system that has a moderate star formation rate, which could be induced by a minor merging event.
