This galaxy presents as an apparent irregular morphology, suggestive of a potential ongoing or recent merger event. The galaxy exhibits a non-uniform luminosity profile, appearing brightest towards what seems to be a central region, though a distinct nucleus is not clearly resolved. A faint, diffuse blueish glow extends beyond the brighter central region, possibly indicating a recent episode of star formation. There are faint features visible that suggests disturbance of the main galactic body. Possible tidal tails or disrupted structures may be present, although low signal-to-noise makes definitive assessment challenging. Overall, the galaxy appears to be a system undergoing gravitational interaction, potentially leading to a merger or significant morphological transformation. The overall color profile seems to indicate a relatively low rate of star formation.
