The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a spheroidal morphology, with a high degree of roundness in its overall shape. There is no evidence of significant spiral arm structure or a prominent disk component. The central region of the galaxy displays a bright, concentrated core, suggesting a high stellar density. The color gradient appears to shift towards redder hues in the core, possibly indicating an older stellar population. The outer regions of the galaxy show a gradual decrease in brightness, lacking distinct features. There is no visual indication of any major merger events or significant tidal disturbances in its immediate vicinity, nor any sign of major star forming activity. The galaxy appears to be a relatively quiescent system.
