The galaxy presents as a relatively smooth elliptical morphology, exhibiting a noticeable central bulge. The light distribution appears concentrated towards the galactic center. The color index suggests a population dominated by older stars, with a subtle reddish hue evident in the outer regions. The galaxy displays a moderate ellipticity. There is some evidence of minor disturbances, potentially indicating past interactions or minor merger activity. The overall structure suggests a system that is relatively relaxed and evolved.
