This galaxy appears to be a spiral galaxy, seen nearly edge-on. A central bulge of older, yellow-white stars dominates the visual appearance and has a significant contribution to the overall luminosity. The disk is relatively thin and elongated, with a faint blueish tinge suggesting ongoing star formation. No distinct spiral arms are clearly discernible given the viewing angle, but the slight variations in color along the disk might suggest underlying arm structures. There is no indication of a recent major merger, though some minor tidal disturbances cannot be ruled out. The galaxy appears to be relatively isolated. The estimated size and luminosity suggest it is a relatively normal spiral galaxy in terms of mass and star formation rate.
