The galaxy presents as an extended, relatively compact object with a somewhat elliptical morphology. It appears to exhibit a smooth overall structure, but with some subtle features that could be interpreted as minor disturbances. A significant portion of the galaxy's light seems to be concentrated towards the center, suggesting a prominent bulge or nucleus. The color distribution indicates a range of stellar populations within the galaxy, with bluer regions possibly indicative of more recent star formation and redder regions suggesting older stellar populations. The galaxy does not appear to be undergoing a major merger, although there is a possibility of some tidal features or subtle irregularities that might suggest past or ongoing minor interactions.
