The galaxy exhibits an elliptical morphology, appearing somewhat elongated but largely smooth in texture. A central bulge is discernible, characterized by a concentrated region of intense yellowish-orange luminosity, suggesting a high density of older stellar populations. Extending outward from the core, the galactic halo displays a more diffuse and fainter glow, with subtle color variations indicating the presence of younger, bluer stars intermixed with older, redder populations. There is a hint of a disk-like structure, but it is not well-defined and possibly disrupted. The overall structure presents minor disturbances and irregularities in the outer regions, possibly indicating past minor merging activity.
