The galaxy presents a largely smooth, elliptical morphology. Its light distribution appears centrally concentrated with a gradual falloff in intensity towards the edges. There is a notable lack of distinct features such as spiral arms or a prominent bulge, supporting the smooth classification. The galaxy exhibits a slightly oblate shape, appearing more "in-between" rather than perfectly round or elongated. No significant tidal disturbances or merging features are obviously visible, suggesting that the galaxy is relatively undisturbed. Color gradients across the galaxy are subtle, with an overall redder hue, implying an older stellar population and lower ongoing star formation activity.
