The galaxy exhibits a disk-like morphology, though the disk appears somewhat amorphous and lacks a well-defined edge. Some features indicate the presence of weak spiral arms extending from the central region. A moderate bulge appears present, contributing significantly to the overall light profile. The galaxy displays a central bar feature, appearing as a subtle elongation across the core region. There appears to be no major ongoing merger event, though a subtle disturbance may be present, possibly indicating a minor interaction in its past. The central region shows a gradient of intensity. The presence of a disk and spiral arm structure suggests recent star formation. The galaxy has an estimated half-light radius of approximately 3.7 arcseconds.
