The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light profile suggests minimal disk features or spiral arms. The core exhibits a high degree of luminosity, with a gradual decrease in intensity toward the outer regions. The color distribution is slightly redder in the central regions compared to the periphery, potentially indicating an older stellar population dominating the bulge. There appears to be no sign of strong tidal interactions or major mergers, although there might be minor irregularities in the outer halo, possibly indicating subtle disturbances. Overall, the galaxy appears to be in a relatively relaxed state of morphological equilibrium.
