The galaxy presents as a somewhat amorphous, irregular structure with a diffuse, hazy appearance. There is a slightly elongated form, suggesting some degree of disk-like morphology, but it's not well-defined. The color gradient appears subtle, with a general bluish hue, potentially indicative of active star formation, yet overall it is rather faint. There may be some internal clumping or knotting suggesting early-stage mergers are possible or perhaps there is starburst activity within the galaxy. Due to the fuzziness, no clear spiral arms or a central bulge is visible, although there may be a faint centrally concentrated region. It is not a symmetrical shape, suggesting some level of gravitational interaction may be occurring.
