The galaxy presents as a centrally concentrated object with a relatively smooth appearance. The core exhibits a bright, yellowish-white hue, indicating a likely concentration of older stellar populations. The galaxy appears somewhat elliptical, with a degree of elongation. There are subtle hints of bluer regions extending from the central bulge, possibly indicative of ongoing star formation within a disk-like structure, or a ring-like structure around the center. There is a minor asymmetry in the disk/halo region, hinting at a possible past interaction or minor disturbance in the galactic structure. The absence of clear spiral arm structure suggests that it might be an early-type spiral or lenticular galaxy viewed at an angle that obscures such features, or possibly a transitioning galaxy undergoing transformation from a spiral to an elliptical morphology. Overall, the galaxy seems to be a massive system with moderate star formation and a relatively quiescent morphological state.
