This galaxy exhibits a generally smooth morphology with minimal discernible disk-like features. The light distribution indicates a centrally concentrated brightness profile with a relatively rapid decline in luminosity moving outwards from the core. It is slightly elongated in shape. The galaxy's color index is observed to shift from slightly redder in the core to bluer colors towards the outer regions. Overall, the light suggests ongoing star formation. There is no visual evidence of strong tidal disturbances, indicating a lack of major recent merger events.
