The galaxy presents a primarily smooth and elliptical morphology. It exhibits a concentrated central bulge that is elliptical, with a gradual fading of luminosity moving outwards. The galaxy is slightly elongated, with a hint of a disk-like structure, however, it lacks distinct spiral arms or well-defined features. A yellow hue dominates the central region, suggesting an older stellar population. Fainter blue fringes are present, indicating some ongoing star formation activity. No signs of strong tidal disturbances or major mergers are readily apparent, although subtle asymmetries suggest a possible minor interaction or past perturbation. The overall structure indicates a galaxy that is relatively evolved.
