The galaxy appears as a diffuse, oblong structure exhibiting a primarily bluish hue, suggestive of ongoing or recent star formation. Its central region is more concentrated, possibly indicating the presence of a galactic bulge. Fainter, less defined regions extend from the center, hinting at a possible disk-like structure. There is some asymmetry apparent, with a faint disturbed region on one side. The galaxy does not appear to be strongly interacting or undergoing a major merger, although minor disturbances cannot be ruled out. The relatively faint and diffuse nature of the galaxy, along with its blue color, could suggest a dwarf galaxy with a lower stellar mass and low rate of star formation.
