The galaxy presents as a somewhat elliptical, relatively smooth structure. A distinct central bulge is observed, displaying a brighter, more concentrated light profile. This central region transitions gradually into a fainter, more diffuse halo. The overall color appears to be slightly blue-tinged, hinting at the presence of some younger stellar populations. There are no immediately obvious signs of spiral arms or significant dust lanes. Minor irregularities in the outer halo suggest possible past interactions or minor disturbances. The general morphology points toward an early-type spiral or lenticular galaxy, possibly in a relatively quiescent state.
