The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge that dominates its overall structure. It shows a gradual fading of luminosity from its core outwards. The color profile suggests an older stellar population. Specifically, the galactic core emits light across the g, r, and z bands, with the emission in the redder bands (r and z) being slightly more prominent compared to the green band (g). This color gradient indicates a population of older, redder stars and a low rate of ongoing star formation. There is no substantial evidence of spiral arm structures or other significant features like dust lanes.
