The galaxy presents as a spiral type, exhibiting a disk-like structure viewed at an angle slightly inclined to our line of sight. Two prominent spiral arms emanate from a central bulge, displaying a morphology characterized by intermediate winding. These arms, traced by regions of bluer light indicative of star formation, appear somewhat flocculent in nature. The central bulge is of moderate size, appearing yellow-white indicating an older stellar population. A bar feature is present and visible across the central region. There is no distinct evidence of ongoing major merger activity. The overall appearance suggests a well-formed, rotating spiral galaxy.
