The galaxy presents a largely smooth, elliptical morphology. The core exhibits a high degree of radial symmetry. A subtle color gradient is observed, transitioning from a reddish hue in the central region to a slightly bluer periphery, suggesting a radial variation in stellar population. No prominent spiral arms or bar structures are discernible. Some minor irregular features appear on the outer edges of the galaxy, suggesting possible minor interactions. Overall, the galaxy seems well-formed with no major signs of significant disturbances.
