The galaxy presents as a centrally concentrated structure, with a primarily smooth morphology. The overall shape appears elliptical, exhibiting a high degree of roundness. There is little evidence of spiral arms or a distinct disk. A subtle color gradient is observable, with a slightly bluer hue in the outer regions transitioning towards a redder core. While largely undisturbed, subtle asymmetries suggest a possible past or ongoing minor interaction. Star formation appears to be present, albeit at a moderate level, as suggested by the blue color.
