The galaxy appears as a centrally concentrated, elliptical-like structure. It presents a relatively smooth morphology, lacking prominent spiral arms or significant irregular features. The color gradient suggests an older stellar population dominating the galaxy's light, with a central, yellowish hue indicating a concentration of evolved stars. There is a subtle blue component present in the surrounding halo, which could suggest the presence of a low level of younger stars on the outskirts. No major disturbances or signs of ongoing mergers are evident, implying a dynamically relaxed system, although subtle asymmetries cannot be ruled out at this resolution. The galaxy exhibits a moderate level of light intensity, appearing neither exceptionally bright nor particularly faint. Its overall shape is close to round, showing limited elongation.
