The galaxy presents as a somewhat elliptical, disk-like structure. A central bulge is visible, appearing bright and concentrated, potentially indicative of an older stellar population. The disk exhibits a relatively smooth texture with hints of spiral structure, though these are not sharply defined. The color profile suggests a mix of stellar populations, with the central bulge appearing yellower and warmer in tone, transitioning to cooler blue hues in the outer regions of the disk. This could indicate ongoing star formation in the periphery. The overall shape indicates the system has likely experienced only minor disturbances to its overall structure.
