The galaxy presents as a relatively smooth and concentrated spheroid. It appears largely featureless, exhibiting no prominent spiral arms or distinct bar structure. The central region displays a high surface brightness, suggesting a dense stellar population or active galactic nucleus. Moving outward from the core, the light profile gradually diminishes, transitioning into a diffuse halo. The galaxy appears to be fairly elliptical. There is no indication of ongoing major mergers or significant tidal disturbances in the immediate vicinity. The galaxy exhibits a color gradient, with a yellower core transitioning to a slightly bluer halo. This could reflect variations in the stellar populations, with older stars dominating the core and younger stars being more prevalent in the outer regions. Overall, the object is consistent with an elliptical galaxy at intermediate redshift.
