The galaxy presents a predominantly smooth morphology, appearing nearly spheroidal in shape. There is no clear evidence of spiral arms or a distinct disk structure. Color gradients are present, shifting from a core that displays a yellowish-red hue, to a more diffuse, slightly bluer outer region. This color distribution suggests a stellar population that is more evolved and redder in the central regions, potentially indicating older stars and a lack of recent star formation there. The blue tinge in the outer parts of the galaxy might indicate regions of ongoing or more recent star formation, although faint. There is no strong indication of any major ongoing merger activity, although a slight irregularity on one side could hint at a past minor interaction. The galaxy appears relatively isolated.
