The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a notable degree of roundness in its overall morphology, with a slight elongation. The central region appears as a bright, unresolved core that gradually fades outwards. The color profile suggests a greater concentration of older stellar populations within the core. The outer regions display a somewhat bluer hue, hinting at the possibility of ongoing, albeit subdued, star formation activity, though this is not visually prominent. There is no evidence of any major merging events or tidal disturbances. The galaxy appears undisturbed and well-formed. No spiral arms or obvious disk structures are apparent. Overall, the galaxy appears to be an elliptical or lenticular galaxy with a large mass. The data suggests suppressed star formation.
