The galaxy presents a smooth, elliptical morphology. The light distribution appears centrally concentrated, with a bright, somewhat compact core. The color profile transitions from a yellowish-orange hue at the center to a slightly bluer tint in the outer regions, suggesting older stellar populations are more prominent in the core with some younger stars present in the arms. There is no discernible spiral structure. The galaxy shows no signs of significant tidal disturbances or ongoing mergers. The round shape of the galaxy indicates it is not cigar shaped.
