The galaxy presents as a centrally concentrated object with a relatively smooth overall appearance, possibly elliptical or lenticular in nature. The central region exhibits a high degree of luminosity, indicating a substantial concentration of stars or an active galactic nucleus. There is little evidence of prominent spiral arms or other distinct features typically associated with disk galaxies. The galaxy's shape is slightly elongated. Some minor perturbations or signs of recent interaction might be present but are not prominent, suggesting a relatively undisturbed morphology. The redder color towards the outskirts could indicate an older stellar population compared to the slightly bluer central region. Based on the observed color and morphology, star formation is probably minimal.
