The object appears to be a relatively smooth galaxy, with a somewhat elliptical morphology. There is a suggestion of some substructure, though the resolution is limited. The light distribution is concentrated towards the center, with a notable color gradient. The central region appears more yellow/orange, suggesting an older stellar population, while the outer regions exhibit a bluer hue, potentially indicative of ongoing star formation. There does not appear to be any strong evidence of a major ongoing merger, although a slight asymmetry in the light distribution might suggest minor interactions or internal disturbances. The overall roundness suggests it is not a strongly barred spiral galaxy seen edge-on. The light seems fairly even across the galaxy, further supporting the smooth classification. The redshift of the object indicates that it is a distant galaxy.
