The galaxy presents a distinct spiral morphology, with two prominent spiral arms emanating from a central bulge. The spiral arms appear well-defined, exhibiting a medium winding pattern. The central bulge appears to be of moderate size compared to the overall disk. There is a suggestion of a bar structure, though not strongly defined. The galaxy is not viewed edge-on, but at a moderate angle, allowing for good resolution of spiral structure. The disk is the dominant feature of this galaxy, and it does not show signs of a major merger or substantial tidal disturbances.
