The galaxy presents as an elliptical morphology, with a centrally concentrated bulge that emits strongly. The overall color profile suggests a predominantly older stellar population with a redder hue, though there appears to be some bluer emission in the outer disk, possibly indicative of more recent star formation. The galaxy displays a fairly smooth light distribution, with minimal signs of strong spiral arm structures or major disturbances. The observed ellipticity suggests a slightly flattened spheroidal shape.
