The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, showing a dominant, spheroidal component. There is some suggestion of a disk-like structure or feature, but it is not sharply defined. The color is slightly bluer in the central regions, implying the presence of a younger stellar population there, surrounded by a more extended, reddish halo. There is no evidence of ongoing major merger activity, although a slight asymmetry suggests a possible minor interaction or disturbance in its recent history. The overall appearance leans toward an early-type galaxy such as an elliptical or lenticular, with little to no prominent spiral arm structure.
