The galaxy presents as a relatively compact, elliptical morphology. It exhibits a smooth, concentrated light profile, suggesting an older stellar population. The color gradient transitions from a yellowish core to a slightly bluer halo. There is no evidence of spiral arms, a bar, or any other disk-like features. There seems to be some interaction with a neighboring blue galaxy or star system. Its roundness suggests we are observing it nearly face-on. There is no clear sign of a major ongoing merger, but there could be some minor disturbances affecting its overall shape. Overall, the galaxy appears to be a passively evolving system with a likely low star formation rate.
