This galaxy presents as a spiral type, exhibiting a notable disk structure. The spiral arms are well-defined, tracing a generally organized pattern from the central region outward. Two dominant arms are visible, demonstrating a fairly consistent winding pattern. The winding appears to be of medium tightness. A bar structure is present across the central bulge region. The bulge itself is moderately sized relative to the disk, with a noticeable central concentration of light, indicating a possible supermassive black hole or nuclear star cluster. There is no indication of the galaxy currently undergoing a major merger event, but the galaxy appears slightly disturbed.
