The galaxy appears to be an interacting system, possibly in the late stages of a merger. Two primary components are visible; a larger, more diffuse body, and a slightly smaller, more compact component with evidence of tidal disruption. The larger component exhibits a yellowish core, with a faint, blueish haze extending outwards. The smaller component appears similar, though more centrally concentrated. There is a distinct plume-like structure extending away from the core, indicating ongoing tidal forces at work within the system. The overall morphology lacks a defined spiral structure, suggesting that any pre-existing disk has been significantly disrupted. The system has a moderate redshift. The stellar population appears mixed, containing both older, redder stars and younger, bluer stars, with ongoing star formation occurring within the galaxy.
