The galaxy exhibits a morphology consistent with an elliptical or lenticular type. Its light profile is relatively smooth, with a high degree of central concentration, appearing largely featureless beyond a slight elongation. The galaxy displays a color gradient, transitioning from a yellowish-white core to more reddish hues in the outer regions. This suggests a stellar population that is dominated by older stars, especially in the outskirts. There are some indications of tidal disturbance and a possible ongoing merger. It also displays signs of moderate star formation.
