The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a diffuse, elliptical morphology, with a gradual decline in surface brightness moving outward from the core. The central region is bright, indicating a high stellar density or an active galactic nucleus. There is a hint of a redder color in the outskirts of the galaxy and a bluer color towards the central region, indicating a possible difference in stellar populations, with older, redder stars dominating the outer regions, and younger, bluer stars closer to the core. No distinct spiral arms or bar structures are readily apparent. Based on the overall smooth appearance, it is likely an elliptical galaxy. The presence of some bluer color in the center suggests that there is some star formation occurring. Overall, the galaxy exhibits only mild disturbances to its overall form, and appears to be a relaxed system.
