The galaxy presents as a mildly elliptical, luminous object with a smooth, relatively featureless appearance. The light is concentrated towards the center, indicating a significant bulge component. The color gradient suggests a potentially older stellar population, with a reddish or yellowish hue dominating the overall light profile. There is very little evidence of prominent spiral arms or dust lanes. Faint disturbances or asymmetries are not visible. The galaxy appears isolated, with no obvious signs of major interactions or mergers.
