The galaxy presents as a generally smooth and rounded structure. A significant concentration of light emanates from the central region, indicating a prominent galactic bulge. The outer regions are less defined, with a gradual fading of light intensity moving outwards. There is little to no indication of spiral arm structures or significant dust lanes. The galaxy exhibits a yellowish hue in its central region, transitioning to a more blueish/green tint in its outer areas. Some subtle disturbances and irregularities may exist on the outer edges of the galaxy, but appear minor.
