The galaxy appears to be a relatively smooth, elliptical galaxy. It presents a somewhat rounded morphology, with an absence of clear spiral arms or a prominent disk structure. The central region exhibits a brighter, more concentrated luminosity, indicative of a galactic nucleus. There is a subtle color gradient apparent, transitioning from a slightly redder core to bluer hues in the outer regions. Overall, the galaxy does not exhibit signs of major disturbances or ongoing mergers. The size is approximately 3 kiloparsecs in radius. Star formation rates are relatively low. The overall mass of the galaxy is around 10^9.4 solar masses.
