The galaxy presents an elliptical morphology, appearing largely spheroidal with a discernible, bright central bulge. There are indications of possible disturbances. A faint, asymmetric halo or arm-like extension appears to emanate from one side of the main galactic body, suggesting possible tidal interactions or recent merger activity. The galaxy exhibits a color gradient, transitioning from a bright, yellow-white core to a fainter, reddish outer region. This suggests potential variations in stellar populations, with older, redder stars dominating the outer regions and younger, hotter stars concentrated within the core. The overall structure is not perfectly smooth, showing some irregularities that further support possible ongoing or past interactions. The outer regions of the galaxy seem diffuse, lacking sharp boundaries.
