The galaxy presents as a centrally concentrated object with a generally elliptical morphology. The core exhibits a bright, yellowish-white hue, indicating a likely population of older stars. The light profile appears smooth, without significant clumpy features or spiral arm structures visible at this resolution. The surrounding galactic disc transitions from the core's yellowish-white to a more diffuse and reddish outer region. This color gradient suggests ongoing or recent star formation in the outskirts of the galaxy. No major tidal disturbances or signs of ongoing mergers are apparent, although there are possible very faint irregularities in the outer halo which could be the result of minor interactions with small objects in the past. The galaxy's overall appearance aligns with that of a relatively evolved system.
