The galaxy presents as a relatively compact and luminous object. Its morphology appears predominantly smooth and rounded, suggestive of an elliptical galaxy or a spiral galaxy viewed face-on with a dominant bulge. There is faint suggestion of a disk component. The galaxy appears to be undergoing or have undergone some sort of disturbance or merging event, evident by the slight asymmetry. The color profile indicates a redder population, suggesting a lack of active star formation and a dominant population of older stars.
