The galaxy presents as a centrally concentrated, lenticular system. It exhibits a dominant, smooth spheroidal component with a noticeable lack of distinct spiral arm structures. The overall shape is elongated, approximately cigar-shaped, suggesting a possible ellipsoidal morphology. There is a slight color gradient visible, transitioning from a relatively bluer outer region to a redder core, which might indicate older stellar populations concentrated towards the center. While the galaxy appears relatively undisturbed in its overall form, there is a hint of minor asymmetry. No prominent tidal tails or major distortions are immediately apparent. This object appears to be in a relatively quiescent state, with limited ongoing star formation.
