The galaxy presents as a relatively smooth, elliptical structure. It exhibits a bright, concentrated central bulge that gradually diffuses outwards, with no apparent spiral arm structures. There is minimal evidence of significant dust lanes or patchy star formation regions. The overall color appears to be a blue/white hue, suggesting a moderate population of younger, hotter stars, although the smoothness implies an older, more evolved stellar population dominates. The galaxy does not show any signs of significant ongoing merger activity or major tidal disturbances, although a slight asymmetry to the light distribution could hint at minor gravitational interactions in its past or present environment. The galaxy appears to be quite round.
