The galaxy presents as a moderately bright, slightly elongated structure. Its core appears relatively smooth and centrally concentrated, with a gradual decrease in luminosity towards the outer edges. There is a suggestion of a disk-like structure. Subtle irregularities or disturbances are observed in the galactic disc, which might indicate minor gravitational interactions or internal activity. The overall color appears relatively uniform, with a slightly yellowish-white hue, suggestive of a population of older stars. There appears to be a fair amount of internal dust as evidenced by the small amount of red extinction that is apparent. There is no clear evidence of strong spiral arms or a prominent central bar.
