The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated morphology with a gradual decrease in luminosity outward from the core. The galaxy possesses a generally round shape, showing minimal deviation from circular symmetry. There's a notable lack of prominent spiral arms, bars, or other distinct features typically associated with disk galaxies. Color gradients suggest a redder core, with stellar populations dominated by older, less massive stars. There is very little indication of ongoing star formation. There is no evidence of a major merger or tidal disturbances.
