The galaxy presents as a centrally concentrated object, exhibiting a relatively smooth morphology. The primary light emission appears yellowish, transitioning to a fainter greenish hue in the outer regions. The overall shape is largely elliptical, verging on circular. There is no clear evidence of spiral arm structures or a prominent disk. Indications are that this is a fairly massive galaxy, the light suggesting the presence of an older stellar population, as well as some degree of current star formation. There are no apparent signs of tidal disturbances or ongoing mergers, indicating that it is likely an isolated system in a fairly quiescent state.
