The galaxy presents a largely smooth morphology, with a relatively featureless appearance at this resolution. The light distribution suggests a centrally concentrated structure. The galaxy exhibits an intermediate ellipticity, appearing neither perfectly spherical nor highly elongated. There is a slight suggestion of minor disturbance in its structure; faint, asymmetric features are possibly present at one end. There is no distinct spiral arm structure or central bar visible. The central region appears brighter than the outer regions, implying a concentration of light and potentially older stellar populations toward the galactic nucleus. The galaxy's color is predominantly blue-green, suggesting the presence of younger, hotter stars.
