The galaxy presents as a relatively compact system. Its overall morphology appears to be relatively smooth and elliptical, with a centrally concentrated luminosity profile. There are no prominent spiral arms or a distinct disk structure visible. The color appears somewhat uniform, with a slight reddening toward the center. Some subtle disturbances or irregularities in its outer regions can be discerned, possibly hinting at minor interactions or past merger events. Overall, the light suggests a relatively old stellar population with low current star formation rates.
