The galaxy appears as a centrally concentrated, smooth, elliptical structure. The light distribution suggests a high degree of symmetry with a gradual decline in surface brightness from the core outwards. The dominant color is yellowish-orange, suggesting an older stellar population. There is no apparent spiral arm structure or significant dust lanes visible. Based on the morphology, the galaxy is consistent with an early-type galaxy, likely an elliptical, with little to no current star formation. Subtle, extended, greenish fringes extend from the galaxy body, possibly indicative of low levels of on-going star formation. Overall, the galaxy exhibits a relaxed, relatively undisturbed morphology.
