The galaxy presents as a spiral type, viewed at an inclined angle. A prominent disk structure is visible, exhibiting well-defined spiral arms. The arms appear tightly wound, tracing a relatively ordered pattern. The galaxy displays a central bulge of moderate size, though it does not visually dominate the overall structure. Evidence suggests a bar feature bisecting the bulge region, exhibiting a noticeable presence. There are no obvious signs of major disturbances or interactions with other galaxies, though minor asymmetry may be present. The color distribution suggests a mix of stellar populations throughout the disk. The overall appearance suggests a relatively massive galaxy, actively undergoing star formation.
