The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a bright, concentrated luminosity profile, suggestive of a significant stellar population. The galaxy appears relatively round, with only a slight deviation from perfect circularity. There is no clear evidence of spiral arms, bars, or other distinct features typically associated with disk galaxies. Faint hints of extended diffuse light suggest a possible halo or envelope surrounding the main body of the galaxy. Overall, it appears to be an evolved system with little ongoing star formation.
