The galaxy presents a moderately elliptical morphology, appearing largely smooth with a concentrated central bulge. The luminosity profile appears to gradually decline from the core outwards. There is some indication of a flattened disk component, however, it is not sharply defined. A subtle color gradient is visible, shifting from a yellow-orange central region towards bluer hues in the outer regions. This color difference may suggest ongoing star formation in the outer regions. There are some faint signs of disturbances in the disc of the galaxy but it is not clear what is causing them. Based on its apparent features, it is most likely a galaxy transitioning from being an elliptical to more of a spiral galaxy.
