The galaxy presents as a relatively compact, centrally concentrated object. Its morphology appears to be smooth, lacking prominent spiral arms or a distinct disk structure. The light distribution suggests a spheroid-dominated system. The color gradient indicates a redder core, potentially composed of an older stellar population, surrounded by a slightly bluer halo, indicative of recent or ongoing star formation. There is no visual evidence of a major ongoing merger or strong tidal disturbances. The overall shape approximates an elliptical form with a high degree of central symmetry. Faint, diffuse light extends from the central region, suggesting a relatively large effective radius.
