This galaxy exhibits a centrally concentrated luminosity profile, appearing elliptical in shape. A bulge component is noticeable. The galaxy shows a relatively smooth appearance, lacking prominent spiral arm structures. The overall color gradient suggests a redder core, likely indicating an older stellar population, with bluer outer regions that potentially mark areas of more recent star formation. The galaxy's morphological classification leans toward an elliptical or lenticular type, based on the smoothness and light distribution. The galaxy is at a redshift of approximately z = 0.073, corresponding to a distance where its light has been stretched by the expansion of the universe.
