The galaxy presents a generally smooth, elliptical morphology. It appears relatively undisturbed, lacking prominent spiral arms or significant tidal features suggestive of recent major mergers. The light distribution is concentrated towards the center, with a gradual decrease in brightness toward the outer regions. The ellipticity is moderate, suggesting a shape somewhere between perfectly circular and highly elongated. The galaxy exhibits a color gradient, transitioning from a slightly bluer hue in the central region to redder colors in the outer halo. This suggests a potential distribution difference in stellar populations, with younger, bluer stars more prevalent in the central region and older, redder stars dominating the outskirts. There is no clear evidence of dust lanes or strong star-forming regions.
