The galaxy appears as a centrally concentrated, relatively smooth object with a nearly circular morphology. Its core exhibits a yellowish-white hue, indicating a population of older stars. There is a subtle color gradient visible, transitioning to a slightly redder shade in the outer regions, which could potentially suggest the presence of a more aged stellar population or dust obscuration. The galaxy lacks any prominent spiral arm structures or significant disturbances, appearing quiescent in nature. Faint extensions surrounding the main body are suspected, though this can be confirmed by further data. Overall, it seems to be an elliptical or lenticular galaxy with a substantial stellar mass and moderate star formation.
