The galaxy appears to be an elliptical or lenticular type, exhibiting a largely featureless morphology. It presents a smooth, centrally concentrated luminosity profile. The shape is moderately elongated, displaying an intermediate ellipticity. The lack of defined spiral arms or dust lanes suggests a relatively quiescent galaxy with little active star formation presently occurring. There are no signs of a major ongoing merger, but a possible minor disturbance might be present in the outer regions. The galaxy's color suggests a population dominated by older, redder stars. The overall structure indicates an evolved system, possibly having exhausted its supply of gas available for star formation.
