The galaxy presents a largely elliptical morphology with a smooth, diffuse appearance. The core region exhibits a high degree of luminosity, fading gradually into the outer regions. There is little to no indication of spiral arm structures or prominent dust lanes. The overall color profile suggests a relatively evolved stellar population, with a higher concentration of older, redder stars within the central bulge. Faint hints of blueish hues are present in the outskirts, indicating a potential presence of younger stars, but at a reduced rate compared to the core. The galaxy exhibits no obvious signs of tidal disturbances, major mergers, or significant asymmetries, suggesting it is a relatively undisturbed system, and hints at a population somewhere between $10^9$ and $10^{10}$ solar masses. Its rate of star formation is low.
