The galaxy presents as a somewhat elliptical structure with a bright, concentrated central bulge. The overall color suggests a mixed stellar population. The core exhibits a yellowish hue, potentially indicative of older, cooler stars. Moving outward from the core, the color transitions into a bluer, somewhat irregular halo. This suggests ongoing or recent star formation regions. The light distribution appears mostly smooth, but there is faint evidence of possible spiral arm structures or tidal disturbances, particularly in the outer regions. The galaxy is relatively compact. There is some indication of low level star formation. Overall, the galaxy appears to be somewhere between an elliptical and a spiral galaxy in terms of morphology, possibly undergoing a transition or having experienced interactions in its past.
