The galaxy presents an elliptical morphology, appearing relatively smooth and featureless. The light distribution indicates a centrally concentrated bulge. The galaxy exhibits a color gradient, transitioning from a yellowish hue in the central regions to a bluer tint towards the outer edges. This may suggest a difference in stellar populations, with older stars concentrated in the core and younger, bluer stars populating the outer regions. The overall shape is elongated, appearing cigar-shaped, suggesting that it is not perfectly spherical. There are no obvious signs of tidal disturbances or major mergers, though minor disturbances cannot be ruled out.
