The galaxy presents a distinct spiral structure, characterized by two prominent arms. These arms exhibit a relatively tight winding pattern, originating from a central, somewhat elongated bulge. The bulge appears moderately sized in relation to the overall disk. A bar-like structure is visible traversing the central region. The spiral arms show subtle variations in color, hinting at ongoing star formation regions. There is no evidence of major merger activity, although there may be some minor disturbances in the outer disk. The galaxy is not observed edge-on; a clear disk structure is visible.
