This galaxy exhibits an elliptical morphology, appearing as a flattened spheroid. The central region displays a concentrated brightness, suggestive of a prominent galactic nucleus. Moving outwards, the intensity gradually diminishes, although the galaxy’s boundary appears somewhat indistinct. There is a slight bluing towards the outer edges which may imply the existence of younger star formations. Overall, the galaxy is fairly smooth with no sharp visible disturbances. It appears to be relatively isolated.
