The galaxy presents as a highly elongated, possibly edge-on spiral or lenticular galaxy. The central bulge appears to be significant, exhibiting a yellow-orange hue suggesting an older stellar population and/or dust obscuration. Extending outwards from the bulge, a faint disk is visible. Hints of blue color in the disk suggest the presence of some younger, hotter stars and potentially ongoing star formation. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. Overall, the galaxy appears to be a relatively massive system with moderate star formation activity.
