The galaxy presents a mostly smooth, elliptical morphology. The central bulge exhibits a concentrated, bright yellowish-white glow, suggesting a population of older stars. The galaxy appears more elongated than perfectly spherical, trending toward a cigar shape. There is a lack of apparent spiral arm structure. Faint, diffuse extensions of the galactic halo are present, fading into the background sky. No major disturbances or merging features are readily apparent, but a slight asymmetry in the outer halo might suggest a minor interaction or disturbance. The overall color profile suggests a relatively quiescent galaxy with a low star formation rate, consistent with its apparent morphology.
