The galaxy presents as an edge-on spiral, or possibly lenticular, system. There is a clear central bulge, appearing bright and yellowish, suggesting an older stellar population. The disk is visible as a flattened structure extending outward from the bulge. The disk appears relatively smooth with faint extensions, indicating a lack of prominent spiral arms. There is a slight blue hue to the outer edges of the disk, possibly from a younger population of stars. The galaxy seems to be relatively undisturbed with no major signs of merging activity or tidal distortions. The bulge has a rounded shape.
