The galaxy presents as a relatively smooth, centrally concentrated structure, likely an elliptical or lenticular type. The light distribution appears quite uniform, with a gradual decrease in intensity from the core outwards. The galaxy is nearly round, showing minimal signs of ellipticity. There is a faint hint of a possible disk-like structure or a bar, but this is not strongly pronounced. No distinct spiral arms or prominent dust lanes are discernible. There's a possible minor interaction or disturbance in the form of slight asymmetry in the outer regions, suggesting a past or ongoing gravitational interaction with a smaller companion. The overall color suggests a mature stellar population, with a bias towards redder wavelengths.
