The galaxy presents as a moderately luminous object at a redshift of approximately 0.1. Morphologically, it appears as a centrally concentrated system with a dominant smooth component. There is little evidence of spiral arms or significant dust lanes. The galaxy exhibits a distinct color gradient, with a redder central region transitioning to bluer outer regions. The shape appears to be somewhere between round and elliptical, with a very slight elongation. There is no readily apparent indication of any major ongoing merger activity, although minor tidal disturbances are not entirely ruled out. Overall, the galaxy seems to be a relatively massive system with moderate star formation, characterized by a spheroid-dominated morphology.
