The galaxy presents as a spiral type, viewed at a slight angle relative to face-on. A central bulge, approximately moderate in size, exhibits a yellowish-orange hue, suggestive of an older stellar population. Two primary spiral arms emanate from the central region, displaying a relatively tight winding pattern. These arms feature a mottled texture, with patches of bluer light indicative of ongoing star formation regions. No significant bar structure is evident. There are slight indications of minor distortions or disturbances in the outer regions of the disk.
