The galaxy presents as a moderately luminous object, appearing yellow-orange in color, suggesting an older stellar population. It exhibits an irregular morphology, possibly indicative of a recent or ongoing merger event. Multiple distinct, bright clumps are visible within the galaxy's structure, with an absence of spiral arm structures or a well-defined disk. There seems to be a tidal tail on the right side, suggesting a merger. The galaxy appears relatively smooth overall, with no strong evidence of active star formation.
