The galaxy exhibits a generally smooth morphology with some indication of a disk-like structure. Its overall shape appears to be more in-between round and elongated, with a slight preference towards a rounded appearance. There is a noticeable concentration of light towards the center, suggesting a central bulge or core. Faint, diffuse extensions can be observed extending outwards. Indications of minor disturbances are present, which may be due to tidal interactions or internal processes. Color gradients exist, with a relatively redder hue in some regions, and a slightly greener hue in the central parts. The galaxy's appearance is not indicative of a major merger event, although subtle signs of ongoing or past interactions cannot be ruled out.
