The galaxy presents as a somewhat elliptical object, exhibiting a smooth, centrally concentrated luminosity profile. The core region is a bright, golden hue, which gradually fades into a less luminous, diffuse halo. The outer regions display a subtle bluish tint, suggesting the presence of a younger stellar population compared to the central core. There is no indication of spiral arm structures or significant dust lanes within this particular image. The galaxy appears well-defined, showing no signs of major tidal disturbances or ongoing merger events. The overall form suggests an evolved system, potentially an elliptical or lenticular galaxy at a redshift of approximately 0.13.
