The galaxy presents a disk morphology with evident spiral arm structures. These arms appear tightly wound around a central bulge. The bulge itself is a moderate size relative to the disk. A faint bar structure appears to be present within the central region, though its definition is somewhat weak. The spiral arms exhibit a mostly two-armed structure, with some uncertainty as to their exact number due to their tightness and indistinct regions. There's no obvious indication of a major merger event, though some minor disturbances or irregularities may be present in the disk structure. Overall, the galaxy's color profile suggests a composite stellar population, with a concentration of older, redder stars in the bulge, and bluer, younger stars within the spiral arms.
