The galaxy presents as a centrally concentrated object with a smooth, relatively featureless morphology. It exhibits a roughly circular appearance, showing minimal deviation from a perfect circle, indicating a low degree of apparent rotational flattening. The galaxy's light is dominated by a yellowish hue in the central region, suggesting an older stellar population. There appears to be a faint greenish halo extending outwards, possibly indicative of a less concentrated distribution of younger stars or ionized gas. There is no discernible spiral structure or bar. The absence of significant morphological disturbances suggests a quiescent history, with no recent major merger events.
