The galaxy presents a generally smooth morphology with a somewhat elliptical shape. It is characterized by a brighter, more concentrated central region, potentially indicative of a galactic bulge. The color profile suggests a moderate amount of star formation activity, particularly within the central region. There may be some minor asymmetries or disturbances in the outer regions, though the overall structure is relatively undisturbed. The color of the core appears to be somewhat redder than the halo, indicating an older stellar population. The galaxy's spatial extent is relatively compact, but resolved in this image.
