The galaxy appears as a roughly elliptical, somewhat smooth distribution of light. The central region exhibits a bright, concentrated core, suggesting the presence of an active galactic nucleus or a dense concentration of stars. The overall color is yellowish-orange, possibly indicating an older stellar population with a lower rate of star formation. There is subtle evidence of slight irregularities or disturbances in the outer regions, which may suggest recent or ongoing minor mergers. The morphology leans towards being largely spheroidal, with a minor fraction showing potential merger activity. The galaxy shows moderate to strong mass, and moderate star formation.
