The galaxy presents as a generally smooth and rounded object, with little discernible internal structure. The central region appears to be more luminous and exhibits a yellowish-gold hue. The light profile decreases in intensity outward, transitioning to a less saturated, greenish halo. No prominent spiral arms, bars, or other features indicative of active star formation are readily apparent. The galaxy exhibits a high degree of symmetry, with a lack of tidal tails or obvious signs of interaction with other galaxies. Minor color variations are seen in the outer halo region, but the overall morphology suggests a system dominated by an older stellar population and quiescent evolution. 
