The galaxy presents as a relatively smooth and centrally concentrated system, likely an elliptical or lenticular type given the absence of prominent spiral arms or dust lanes. The light profile appears centrally bright, with a gradual decrease in intensity towards the outer regions. There is a slight asymmetry in the overall shape, hinting at a possible recent interaction or merger event. The galaxy exhibits a yellowish-red color indicative of an older stellar population and a cessation of significant star formation. The core shows a high degree of roundness. A very faint disk is noted to be at the edges of the galaxy, and a small amount of disturbance is present in the morphology.
