The galaxy appears as a centrally concentrated object with a smooth, relatively featureless morphology. Its overall shape approximates a slightly elongated spheroid. The color profile indicates a higher concentration of light in the redder bands, with a gradual decline towards bluer wavelengths, suggesting an older stellar population and reduced current star formation activity. There is no apparent spiral structure or distinct disk component visible. There is no indication of a strong tidal interaction or significant morphological disturbance. Overall, the object presents as a quiescent galaxy, likely of substantial mass.
