The galaxy presents a centrally concentrated morphology, likely an elliptical or lenticular type. The light is dominated by a yellowish hue, suggesting an older stellar population, with minimal recent star formation. The galaxy is relatively smooth in appearance, exhibiting a high degree of rotational symmetry. There's a hint of disturbance in its form, perhaps due to minor tidal interactions or a past merger event. The estimated size indicates this is a sizable galaxy, with a relatively high stellar mass.
