The galaxy appears to be a relatively compact and luminous elliptical galaxy. It exhibits a smooth, largely featureless morphology, with a high degree of central concentration. The light distribution suggests an elliptical or spheroidal shape, being somewhere in-between perfectly round and slightly elongated. There is no apparent spiral arm structure or significant dust lane obscuration, lending to a uniformly distributed light profile across the galaxy's surface.

The galaxy's color is overall reddish, suggesting an older stellar population dominated by evolved stars. The overall red color is not significantly offset, and there are no distinct features like blue knots that would indicate very recent star formation. This indicates that the galaxy's star formation rate is likely low, or suppressed. There is no apparent evidence of any major ongoing merger activity or strong tidal disturbances, suggesting that it has reached a stable state, or recently experienced a minor disturbance. Overall, this galaxy appears to be a passively evolving system with little ongoing star formation and a well-mixed stellar population.
