The galaxy presents as a relatively compact object with a moderate degree of internal structure. There is a suggestion of a flattened, disk-like component. The color gradient across the galaxy indicates the presence of varying stellar populations, with the central region appearing bluer, suggesting more active star formation or a younger stellar population compared to the redder outer regions. A faint, diffuse halo might surround the primary structure but is difficult to fully confirm due to the image noise and limited resolution. There is a hint of a possible tidal feature. A visual inspection suggests the object's morphology is not entirely smooth.
