The galaxy presents a largely featureless, elliptical morphology. Its light profile is centrally concentrated, indicating a significant bulge component. The galaxy exhibits a smooth texture without apparent spiral arms or dust lanes. It is nearly round, and a slight asymmetry may be present. The core of the galaxy displays a yellowish hue, suggesting an older stellar population, while the outer regions appear slightly bluer, implying the presence of some younger stars or a low level of ongoing star formation. No signs of significant tidal disturbances or interactions with neighboring galaxies are evident.
