The galaxy presents as a centrally concentrated, relatively smooth object with a diffuse, elliptical morphology. Its light profile increases towards the center, indicative of a large bulge component with lower star formation. The galaxy appears to be an early-type galaxy, likely an elliptical or lenticular, based on its overall form and lack of discernible spiral structure or strong star-forming regions. There is a very slight elongation suggesting the object is in between round and cigar shaped. The color indices suggests that the galaxy is redder than the Sun (G-R is 0.64, R-Z is 0.45), indicative of a population of older stars. The galaxy appears undisturbed without any visual signs of interactions or major disturbances.
