The galaxy presents as an irregular, somewhat diffuse structure. Its color is predominantly blue, suggesting recent or ongoing star formation. There appears to be some evidence of disruption, perhaps due to a minor merger or tidal interaction, which could be the trigger for the star formation activity. The galaxy lacks a distinct central bulge or spiral arm structure. Faint extensions or tidal tails may be present but are not well defined due to the galaxy's apparent faintness and diffuse nature. Overall, the galaxy seems to be a relatively low-mass, actively star-forming system undergoing some form of interaction or disturbance.
