The galaxy presents a primarily smooth morphology, with a bright central bulge indicative of a high concentration of stars. A faint, extended disk component appears to surround the bulge. The galaxy exhibits a moderate ellipticity, appearing somewhat elongated in shape. There's subtle evidence of some disturbance of the morphology, though it appears relatively undisturbed and lacks the characteristics of major mergers. The galaxy displays a color gradient, with the central bulge appearing whiter compared to the bluer outer regions, potentially indicative of ongoing or recent star formation in the disk. Based on the color and overall structure, the galaxy is likely a late-type spiral galaxy, likely with a relatively lower-mass.
