The galaxy presents as a single, concentrated object with an elliptical morphology. Its light profile is smooth, displaying a centrally concentrated bulge that decreases gradually in intensity towards its edges. The galaxy exhibits a yellowish hue, suggesting a population of older stars with lower star formation rates. There is no clear indication of spiral arm structures or significant dust lanes. Minor disturbances or tidal features are not apparent, suggesting that it is not currently undergoing a major merging event. The galaxy appears well-defined, with a generally round shape, although not perfectly circular.
