The galaxy presents an overall elliptical morphology, though with a slight asymmetry. The light distribution is centrally concentrated, showing a smooth, featureless structure with no apparent spiral arms or bar. The central region exhibits a bright, diffuse core. The galaxy appears to be relatively isolated, showing no obvious signs of tidal interactions with nearby galaxies. The color gradient appears to shift from a more reddish hue in the core to a bluer color in the outer regions. This suggests an older stellar population in the center, with younger, bluer stars populating the outskirts. The overall form and color distribution implies a galaxy that has largely ceased active star formation, with the remaining star formation concentrated in the outer regions. However, weak star formation may still be present at a low level. A mild disturbance seems to be present, potentially resulting from a past merger event, or a less massive ongoing merger.
