The galaxy presents a somewhat diffuse appearance, with a non-uniform distribution of light. A clear central bulge is not easily discernible. There appears to be a slight elongation, indicative of a potentially disk-like component, though this is not sharply defined. Color gradients are present; the core region exhibits a yellower hue, which could indicate an older stellar population. The outer regions of the galaxy appear bluer, suggesting the presence of younger, hotter stars. There is potential evidence of a minor disturbance or merging event, manifested in the asymmetry of the outer regions, but further investigation is needed to confirm this. The overall structure appears relatively smooth, however, the faintness and lack of sharp details hinder a precise morphological classification.
