The galaxy presents a centrally concentrated morphology, with a generally smooth appearance. The galaxy appears to have a flattened, disc-like structure, though any spiral arm features are faint or unresolved. There is some color variation across the galaxy, potentially indicating differences in stellar populations or dust content. The central region exhibits a slightly brighter and bluer hue, possibly indicative of ongoing or recent star formation. The galaxy's outer regions fade gradually into the background sky, implying a diffuse halo or extended stellar distribution. There is a slight asymmetry, which could potentially indicate the presence of tidal interactions.
