The galaxy appears as an elongated, disk-shaped structure with a smooth and centralized light distribution. It exhibits a yellowish-white hue, suggesting an older stellar population. There's a subtle color gradient across the galaxy, the central bulge region is slightly brighter and yellower compared to the outer disk. Based on the lack of distinct spiral arms, the galaxy is potentially a lenticular or elliptical type. The shape is noticeably elongated, approximately three times as wide as it is tall. There are no obvious signs of active galactic nuclei or major mergers, the galaxy appears to be relatively undisturbed.
