The galaxy presents a generally smooth and rounded morphology. The light distribution suggests a centrally concentrated structure, with a gradual decrease in luminosity outwards. The central region appears brighter and slightly bluer in color, indicating a potential concentration of younger stars or ongoing star formation. A faint, diffuse halo extends beyond the central bulge, lacking defined spiral arms or prominent features. There is a slight elongation in the galaxy's shape, deviating from a perfect circular form. The overall impression is that of a relatively undisturbed galaxy, without strong signs of recent mergers or tidal interactions, although subtle disturbances cannot be ruled out.
