The galaxy appears as a centrally concentrated object, with a smooth and relatively featureless morphology. The light profile suggests a bulge-dominated system. There's a slight elongation, but it's mostly round. No distinct spiral arms or bar structures are readily apparent. The galaxy exhibits a color gradient, with a bluer hue toward the core and a gradual shift to redder tones in the outer regions. The absence of prominent dust lanes further supports the smooth classification. There is no evidence of ongoing major merging activity.
