The galaxy presents as an elliptical morphology, with a smooth and centrally concentrated luminosity profile. The core exhibits a bright, almost stellar-like appearance. The overall color index appears to be relatively red, suggesting an older stellar population with lower ongoing star formation. There is a slight elongation in shape, but the galaxy is generally rounded. No significant dust lanes or spiral arm structures are discernible. There are no obvious signs of major mergers or tidal disturbances, with only a slight indication of a possible minor interaction based on the subtle asymmetry of the outer isophotes. The overall appearance suggests a massive galaxy, passively evolving.
