The galaxy presents as an elliptical-like structure, exhibiting a generally smooth appearance with a concentrated central bulge. The object demonstrates a diffuse, hazy halo, suggesting a lower density of stellar populations at the periphery. The galaxy's form is predominantly spheroid with hints of disk-like features but not pronounced. There is evidence of minor disturbances of the light distribution indicating potential interactions. Color gradients within the galaxy reveal subtle variations, with a somewhat bluer tone near the center compared to the slightly redder outer regions.