The galaxy appears to be a relatively bright, centrally concentrated object with a generally smooth morphology. It exhibits a noticeable color gradient, transitioning from a yellowish-white core to a bluer, fainter outer region. The core displays an approximately round shape, with some slight deviations suggesting a possible departure from perfect ellipticity. The outer regions show some suggestion of a disk like structure. There is subtle evidence of disturbances to the structure of the galaxy, and there may be on going minor mergers influencing its shape. The galaxy shows signs of ongoing, though not particularly vigorous, star formation within its structure. Overall the galaxy is a fairly massive system, situated at a moderate cosmological distance.
