The galaxy presents as a concentrated, centrally bright object, appearing relatively smooth in overall structure. The morphology suggests an elliptical galaxy, or potentially a spiral galaxy seen face-on at a great distance with a significant bulge component. A second, smaller object to the left is interacting with the larger galaxy, and the larger galaxy is not spherically symmetric, suggesting a possible interaction. It exhibits a color profile that is redder in its core and gradually transitions to slightly bluer tones in its outer regions. The presence of these color variations hints at differing stellar populations across the galaxy, with possibly older, redder stars dominating the central regions. There are faint indications of tidal features or other disturbances in the galaxy's outskirts, further suggesting possible gravitational interactions with another galaxy, though more data would be needed to confirm. Overall, the galaxy is relatively compact and lacks obvious signs of significant ongoing star formation.
