The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that is bright yellow, suggesting a population of older stars, likely a lack of significant ongoing star formation. There is a slight elongation to the galaxy's shape, but it appears largely round. No distinct spiral arms or dust lanes are discernible in the image. There is some slight color variation in the outer regions. Based on the object's morphology, it does not show any signs of a major merger or significant disturbance. The light distribution implies a fairly uniform stellar population with little evidence of recent star formation.
