The galaxy presents a smooth, elliptical morphology. It displays a concentrated central bulge that exhibits a yellowish-white hue, suggesting a population of older stars. The outer regions of the galaxy fade gradually, with a slightly bluer color, possibly indicating the presence of some younger stars or ongoing, but weak, star formation. The overall shape is elongated and cigar shaped, lacking any distinct spiral arm structures or prominent dust lanes. The galaxy does not show obvious signs of recent merging activity, such as tidal tails or significant distortions in its overall structure.
