The object appears to be a spiral galaxy at an estimated distance, characterized by a redshift of approximately 0.23. It presents a prominent disk structure with well-defined spiral arms. Two dominant arms are discernible, exhibiting a medium winding pattern. The central bulge is of moderate size relative to the overall disk. There is evidence of a bar structure, possibly weak. The spiral arms display some irregularity, suggesting minor gravitational interaction or disturbance. The galaxy's color profile is consistent with ongoing star formation, particularly within the spiral arms. The overall morphology does not indicate a major ongoing merger, but subtle irregularities suggest potential minor interactions. The galaxy presents a notable disk structure with spiral arms.
