The galaxy presents a largely smooth morphology, appearing nearly elliptical in shape. A dominant central bulge exhibits a yellow-orange hue, indicative of an older stellar population. Fainter, bluer light is observed towards one edge of the galaxy, possibly representing a region of more recent star formation or a tidal feature. There appears to be a companion galaxy to the left, it is unknown whether they are undergoing a merger, but it seems they are close enough to be gravitationally bound. The overall appearance suggests an evolved system with a relatively low star formation rate, transitioning towards a quiescent state. Some asymmetries may be present, hinting at possible past interactions or internal disturbances. 
