The galaxy presents as a fairly smooth, centrally concentrated object, elongated along one axis. Its core appears bright and yellowish-white, suggesting an older stellar population. A faint, diffuse, and slightly bluer disk component is visible extending outwards from the core along the major axis. No distinct spiral arm structures or significant dust lanes are readily apparent. The overall appearance is consistent with that of a lenticular galaxy, possibly transitioning towards an elliptical morphology. There is no strong evidence of ongoing major merging activity, though some minor asymmetry in the outer regions cannot be ruled out.
