The galaxy presents a predominantly smooth morphology, appearing as an elliptical or lenticular type based on its shape. The light distribution appears concentrated towards the center. The galaxy exhibits a slight elongation in its structure, with a color gradient transitioning from a yellowish core to a subtle blueish outer halo, suggesting a population of older stars in the center and possibly some younger stars in the outer regions. There is no evident spiral structure or strong dust lane. There is a very subtle distortion in the shape of the galaxy, but no major interactions are apparent.
