The object presents as a spiral galaxy, viewed at an oblique angle. Its apparent morphology suggests the presence of a central bulge, though not a particularly dominant one. A disk structure is evident, characterized by well-defined spiral arms. The spiral arms appear to be wound rather loosely, with possibly two main arms discernible. There's a hint of a bar-like structure across the central region. Color variations within the galaxy suggest differing stellar populations and regions of active star formation within the disk, displaying bluer hues along the spiral arms compared to the yellower central bulge. The general structure appears somewhat distorted, indicating a possible minor interaction or disturbance.
