The galaxy presents as a slightly elongated, disk-shaped structure. Its color appears to be primarily bluish-white, suggesting a significant population of relatively young, hot stars. There is a subtle color gradient from the core to the edges, with the central region exhibiting a somewhat yellower hue. This could be due to a higher concentration of older stars, dust obscuration, or potentially a weak active galactic nucleus. The overall smoothness of the light distribution indicates that the galaxy is likely an early-type spiral or a lenticular galaxy, possibly viewed at a high inclination. While there are no prominent spiral arms clearly visible, the disk exhibits some irregularities in its outer regions, hinting at possible minor disturbances or interactions with smaller galaxies. The edges of the galaxy are somewhat diffuse, fading gradually into the background sky, which might be attributed to the presence of a faint stellar halo.
