The galaxy appears to be elliptical in shape, exhibiting a smooth morphology with little evidence of spiral arms or other distinct features. The color profile suggests a dominant population of older stars, evidenced by a reddish-yellow hue concentrated towards the core. There are hints of bluer regions, potentially indicating regions of more recent, though limited, star formation. The galaxy displays no obvious signs of a major ongoing merger, although subtle asymmetries might suggest past interactions or minor disturbances. The light distribution appears relatively concentrated, with the majority of the luminosity emanating from the central region.
