The galaxy presents as an edge-on disk galaxy. It exhibits a prominent central bulge, which appears yellowish, possibly indicating an older stellar population. The disk component is relatively thin and elongated, with a blueish tint, suggesting the presence of younger, hotter stars and ongoing star formation. There is no obvious evidence of a strong spiral structure or significant dust lanes within the disk. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal disruptions. Its overall morphology suggests a relatively evolved system undergoing moderate star formation. The size of the galaxy seems to be relatively large and very far away, with a smooth general shape. 
