The galaxy presents a generally smooth morphology, appearing as a diffuse, centrally concentrated object. There is faint suggestion of a disk. The primary color is bluish, with subtle variations indicative of regions with differing stellar populations. The object does not show any clear spiral arm structure or a well-defined central bulge. The faintness and color suggest that the object may be relatively distant, and the light might be faint or blueshifted due to movement of the galaxy relative to Earth. The irregular shape could indicate either a galaxy undergoing a merger, a peculiar galaxy with no distinct morphology, or a disk galaxy viewed at an oblique angle. Low level disturbances in the light surrounding the main galactic structure suggests a potential interaction or tidal features. The relatively small angular size and low surface brightness make detailed morphological classification challenging.
