The galaxy presents a roughly elliptical morphology, elongated along a major axis. The central region displays a higher surface brightness, suggesting a concentration of stellar mass and potentially a bulge component. Fainter and bluer regions extend outwards from this central area, indicative of ongoing or recent star formation activity within a disk-like structure. The galaxy appears to be experiencing some degree of disturbance, with asymmetry suggesting a possible interaction or minor merger event in its past, which may be inducing the observed star formation. Overall, the galaxy seems to have characteristics of a late-type spiral galaxy undergoing some disturbance or transitioning into an elliptical one.
