This galaxy presents as a spiral type. The morphology reveals a central bulge region that appears of moderate size, surrounded by a flattened disk structure. Two spiral arms are distinctly observed emanating from the central bulge. The arms demonstrate a loose winding pattern. Evidence of a bar structure is noticeable spanning through the bulge region. Star formation appears to be active, but not remarkably vigorous. Overall, there is no indication of any ongoing major merging events. The light emitted suggests an intermediate redshift value.
