The galaxy presents as a singular, relatively smooth object. Its overall shape is somewhat elliptical, tending towards round rather than elongated. A centrally concentrated bulge dominates the galaxy's morphology, exhibiting a bright yellowish-white core that gradually fades into the surrounding halo. There is little visible evidence of spiral arm structure or significant disk features. The galaxy exhibits a smooth texture, lacking prominent features like dust lanes, knots of star formation, or tidal tails suggesting major mergers. Minor asymmetry or subtle disturbances may be present, but they are not prominent. The color gradient suggests an older stellar population within the bulge and potentially in the surrounding halo.
