The galaxy presents an elliptical morphology with a flattened profile. A significant portion of the galaxy's light is concentrated in a central bulge region, which exhibits a bright, almost point-like core that is bluer in color, possibly indicating recent star formation. The extended galactic halo shows a smoother, more diffuse light distribution with redder hues, suggesting an older stellar population. A fainter, more irregular feature appears as an extension to one side of the main body, which may indicate a tidal interaction or ongoing merger. The orientation of the galaxy allows for only a limited view of its internal structure.
