The galaxy appears to be a relatively compact system. It exhibits a smooth, elliptical morphology, with a bright, concentrated central bulge. The color gradient suggests a radial change in stellar populations, with the core exhibiting a yellowish hue, possibly indicating an older stellar population. The outer regions have a bluer tint, suggestive of ongoing or recent star formation. There's a slight hint of asymmetry or a very faint tidal feature in the outer halo region, which might indicate past interaction or merger. The galaxy presents with a central region which dominates the light and appears to have a spheroidal distribution. It is observed at a redshift, indicating that it is fairly distant.
