The galaxy presents as a centrally concentrated object, with a smooth, elliptical morphology dominating its structure. The light profile appears regular, lacking any prominent spiral arms or bar features. The core exhibits a bright, yellowish hue, suggesting a significant population of older stars, which dominates the light output in this region. There is evidence of recent star formation, based on the redness around the yellow central core, but the overall star formation rate appears to be low. The galaxy does not appear to be undergoing any major merger events, although there is a slight asymmetry in the outer halo.
