The galaxy presents as an elliptical or lenticular type, displaying a smooth, featureless morphology. It exhibits a moderate degree of ellipticity, appearing neither perfectly spherical nor highly elongated. The color profile indicates a dominance of older stellar populations, with a yellowish-red hue suggesting lower levels of ongoing star formation activity. There is a presence of an apparent merging event occurring with another galaxy, but the system is mostly undisturbed. The galaxy appears to have a high mass estimate.
