The galaxy appears as a centrally concentrated object with a smooth morphology. It is elliptical in shape, but tending towards a round profile. The central region exhibits a bright, yellowish-white color, suggesting an older stellar population. Fainter, bluer light surrounds the core, forming a halo. There appears to be little evidence of spiral arm structure or dust lanes, indicating a more evolved system. No significant tidal features or signs of a major ongoing merger are visible. There are hints of minor disturbances or slight asymmetry, but the overall structure is relatively undisturbed.
