The galaxy appears as a moderately luminous, relatively compact object. It presents with a smooth, largely featureless morphology, suggestive of an elliptical or lenticular galaxy. There is a subtle color gradient observed, with the central region exhibiting a slightly yellower hue compared to the outer regions, possibly indicating a population of older stars concentrated towards the core. There is no visual evidence of spiral arm structure or significant dust lanes, nor any strong evidence of tidal disturbances or ongoing mergers. The overall impression is that of a well-defined, undisturbed galaxy, likely at a moderate redshift.
