The galaxy appears to be a relatively smooth, centrally concentrated system. Its overall color is slightly bluer in the center, fading to redder hues in the outer regions. There is no obvious spiral structure or dust lanes visible. The light profile suggests an elliptical or lenticular morphology, with a high degree of central symmetry and little to no evidence of recent major mergers or tidal disturbances. There is a very slight irregularity that may indicate the remnants of a minor disturbance.
