The galaxy presents as a spiral type, exhibiting a disk structure that is neither perfectly face-on nor edge-on, but at a moderate inclination. Two prominent spiral arms emanate from the central region, displaying a relatively tight winding pattern. A weak bar structure appears to be present in the galactic center. The central bulge is of moderate size, contributing significantly to the overall luminosity. The galaxy does not show any major signs of disturbance or ongoing merging activity, although there are subtle indications of minor asymmetries, suggesting the possibility of past interactions or internal dynamics at play. Star formation appears to be occurring, as evidenced by the bluer hues present in the spiral arms.
