The galaxy presents as a centrally concentrated object with a smooth, relatively featureless appearance. It exhibits a near-circular morphology and has a distinct yellowish hue, suggesting a population of older stars. There is no evidence of spiral arms or a well-defined disk structure. The galaxy does not appear to be undergoing any major merging activity or significant tidal disturbances. The light distribution smoothly diminishes from the center, indicating a relatively even stellar density gradient.
