The galaxy presents as a centrally concentrated object with an apparently smooth morphology. The overall shape is elliptical, with a high degree of roundness. The central region exhibits a high surface brightness, appearing bright yellow-orange. There is no clear evidence of spiral arms, dust lanes, or a prominent disk structure. Faint extensions, or tidal features, are possibly present, but the image resolution limits definitive identification. There is no strong indication of an ongoing major merger event. There is a slight asymmetry in the light distribution which may indicate a minor disturbance. The galaxy appears to be relatively isolated in this field of view.
