The galaxy presents as a relatively smooth, elliptical or lenticular structure with a dominant central bulge. There is a hint of a surrounding disk. The galaxy displays a yellowish-orange hue, suggesting an older stellar population with minimal ongoing star formation. There is a lack of prominent spiral arm structures. Morphologically, it appears fairly regular, although there is some evidence of tidal disruption or a merger event, possibly a minor disturbance in the overall structure. The galaxy exhibits a smooth light distribution, but there are some subtle asymmetries present, potentially indicating a past interaction.
