The galaxy presents as a single, largely homogenous structure. The light profile appears smooth and concentrated, with a high degree of central symmetry, appearing nearly round. There is a slight color gradient from the center outward, with the innermost region exhibiting a yellow-white hue, transitioning to a slightly redder tone in the outer regions. There is no obvious spiral arm structure or distinct bulge component. There may be minor disturbances or tidal features, but the features are subtle. Overall, the galaxy appears as an elliptical or lenticular galaxy, consistent with a relatively old stellar population. The estimated redshift suggests that it is at a moderate distance, and therefore observed at a relatively early stage in its evolutionary history.
