The galaxy presents a generally smooth, elliptical morphology. A bright, concentrated nucleus is apparent, surrounded by a more diffuse, spheroidal halo. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct features. The galaxy exhibits a subtle color gradient, transitioning from a yellowish core to a slightly bluer outer region. There is no obvious evidence of significant dust lanes or recent major merger events. Based on its appearance, it seems the galaxy is a relatively massive system dominated by an older stellar population, with perhaps a low level of ongoing star formation in the outer regions.
