The galaxy appears as a single, concentrated mass of light. The object is elliptical in shape, with a smooth, diffuse appearance. There are no readily apparent spiral arms or other features to suggest a disk-like structure. The central region shows a high concentration of light, with the color tending towards yellow, suggesting an older stellar population and a paucity of ongoing star formation. The outer regions fade gradually into the background, consistent with a relatively old stellar population. There are no indications of tidal tails or other signs of a recent merger event. The overall morphology is consistent with that of an elliptical galaxy with a population of older stars.
