The galaxy appears as a relatively smooth, elliptical structure with a prominent, bright central bulge. The light distribution suggests a high degree of radial symmetry, although it is not perfectly circular; there is a subtle elongation. The overall color is yellowish-white, which is characteristic of older stellar populations. The outer regions of the galaxy fade gradually, indicating a diffuse halo component. There is no obvious evidence of spiral arms or prominent dust lanes. Faint, mottled features may be present in the outer regions, but they are not well-defined. The galaxy does not show any signs of significant tidal disruption or interaction with neighboring galaxies. Based on these features, this object is likely an early-type galaxy, specifically an elliptical galaxy with a large, quiescent stellar population. The inferred mass is substantial, with a low star formation rate.
