The galaxy presents as a centrally concentrated, relatively smooth elliptical galaxy at a redshift of approximately 0.0845. It exhibits a high degree of radial symmetry, lacking any readily discernible spiral arm structures or prominent dust lanes in this imaging. The galaxy appears nearly circular, with only a slight elongation visible. The luminosity profile indicates a strong central bulge that decreases gradually with increasing radius. Color gradients suggest that the core of the galaxy is bluer than the surrounding regions. There is some evidence of a minor disturbance on the left side of the galaxy. There is no apparent ongoing major merger activity.
