The galaxy presents as a somewhat elliptical structure with a central bulge that appears to be a yellow-orange hue, potentially indicating an older stellar population dominating the core. The disk component, while present, is less defined, exhibiting a fainter greenish tint, which could be indicative of some ongoing star formation. The galaxy displays a generally smooth appearance, lacking prominent spiral arms or strong dust lanes. There is no obvious indication of any major merger events, although a minor asymmetry in the outer regions might suggest a past interaction or disturbance. The galaxy's overall morphology suggests it is an intermediate type, possibly an early-type spiral or lenticular galaxy.
