The galaxy presents as a centrally concentrated elliptical with a smooth morphology, exhibiting a bright, yellowish core indicative of an older stellar population. The galaxy appears relatively undisturbed, with a high degree of roundness and no prominent spiral arms or bar structures. A slight elongation is observable. Faint blue tinges at the edges suggest the possibility of some limited ongoing star formation. No signs of significant tidal disturbances or mergers are immediately apparent, although there may be a galaxy nearby. Overall, the galaxy appears to be a relatively quiescent, evolved system.
