The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, yellowish-orange hue, suggesting an older stellar population. Surrounding this core, a faint, diffuse, and somewhat bluer halo is visible. There is no apparent spiral structure or distinct disk, but instead there are subtle color variations within the outer halo. Overall the galaxy shows a smooth appearance with only slight disturbances. The overall morphology is indicative of a quiescent system with moderate star formation activity. The galaxy appears to be relatively isolated, with no immediately obvious signs of ongoing major merger activity. The central bulge dominates the overall light profile.
