The observed galaxy presents a largely smooth, rounded morphology. The light distribution appears centrally concentrated with a gradual falloff in intensity towards the outer regions. There is some evidence of a slightly elongated or ellipsoidal shape, though the overall form is primarily spherical. The galaxy's color is primarily greenish in the image, with an absence of any evident disk structure or spiral arm features. There is no obvious sign of major disturbances, such as tidal tails or multiple nuclei, which could be indicative of an ongoing or recent major merger event. However, there is a possible slight asymmetry in the outer regions, which might suggest a minor interaction or internal disturbance. Overall, the galaxy seems to be a relatively undisturbed system.
