This galaxy presents as a highly elongated disk galaxy, viewed nearly edge-on. The central bulge appears prominent and exhibits a yellowish-orange hue, suggesting an older stellar population. Extending outwards from the bulge, the disk appears relatively smooth with hints of faint, diffuse blue regions, potentially indicating areas of recent star formation. The disk is thin, displaying a notable dust lane along its major axis that bisects the galaxy's light. The overall structure implies a relatively high degree of organization with a well-defined plane, characteristic of mature disk galaxies. There are no obvious signs of major interaction or disturbances visible within the galaxy's morphology.
