The galaxy presents as a relatively smooth, centralized structure, most likely an elliptical galaxy. Its core exhibits a bright, concentrated luminosity, indicative of a high stellar density or possible AGN activity. Moving outward from the core, the light gradually diminishes, forming a smooth, elliptical halo. There are subtle color gradients, with a suggestion of bluer hues on the periphery, possibly reflecting ongoing, though subdued, star formation in the outer regions. The overall morphology is largely undisturbed, with no major tidal features or signs of ongoing major merger events. However, there may be some minor asymmetry visible suggesting a minor interaction. The galaxy is moderately massive, with moderate ongoing star formation and a red shift of around z=0.24. The galaxy is approximately 7 kpc across in physical size.
