The galaxy presents as a centrally concentrated elliptical system. It exhibits a smooth, diffuse light profile with a high degree of symmetry. The core is bright and yellowish, suggesting an older stellar population dominating the central region. Progressing outward, the luminosity gradually decreases, transitioning to a redder hue in the outer regions. There is a notable absence of distinct spiral arms, bars, or prominent dust lanes. The overall morphology implies a galaxy that has undergone significant dynamical relaxation, indicating a relatively quiescent state with potentially low current star formation activity. No signs of major mergers or tidal disturbances are readily apparent.
