The galaxy presents an elliptical morphology. Its shape is moderately elongated, with the major axis noticeably longer than the minor axis. The central region is characterized by a high surface brightness, appearing as a bright, concentrated core, suggesting a significant stellar density. Progressing outward from the core, the surface brightness gradually diminishes, forming a smooth, diffuse halo. The color profile indicates a generally red hue, characteristic of older stellar populations and a relatively quiescent star formation rate. A slight asymmetry can be observed in the outer regions, potentially indicating past interactions or minor disturbances, although no strong tidal features are apparent. Overall, the galaxy appears as a mature, relatively undisturbed elliptical system.
