The galaxy presents as a relatively smooth, elliptical or lenticular structure with a dominant central bulge. The light profile appears concentrated, with a noticeable decrease in surface brightness moving outward from the core. The color is consistent with an older stellar population, appearing reddish-yellow. No distinct spiral arms or significant dust lanes are visible. There is no evidence of any major ongoing merger events, although minor tidal disturbances or faint stellar streams cannot be ruled out without higher resolution data. The overall morphology indicates a mature galaxy that has largely exhausted its gas supply and experiences little active star formation.
