The galaxy presents a centrally concentrated morphology, with a smooth, diffuse appearance dominating its structure. The light profile suggests a spheroidal or elliptical shape. The galaxy's core region exhibits a significantly higher surface brightness compared to its outer regions, indicating a possible concentration of older stellar populations or a supermassive black hole at the galactic center. There appears to be a possible tidal tail or minor merging partner to the lower right. Overall, the galaxy is relatively isolated and appears to be in a more advanced stage of evolution, having largely exhausted its supply of gas and dust, resulting in low levels of star formation.
