The galaxy presents as a moderately inclined, disk-shaped structure. It exhibits a smooth appearance, with a bright, concentrated central bulge. The outer regions of the galaxy are less defined, showing a gradual decrease in luminosity. The color distribution indicates a relatively uniform stellar population throughout the galaxy, with a slight reddening towards the central bulge, likely indicative of older stars or dust obscuration. There is no clear evidence of spiral arm structure or significant star formation regions from this observation. The axial ratio suggests it may be a barred spiral or elliptical galaxy viewed at an angle. Overall, the galaxy appears to be a relatively evolved system, with ongoing, but moderate star formation.
