The galaxy presents as a highly elongated, cigar-shaped morphology, likely an edge-on spiral or a lenticular galaxy. It exhibits a smooth overall appearance, with a central bulge that appears slightly brighter and more diffuse than the disk. The color gradient suggests a redder core, possibly indicative of an older stellar population concentrated in the bulge. The outer regions of the galaxy appear bluer, suggesting the presence of younger, hotter stars in the disk. There are no obvious spiral arm structures visible, reinforcing the possibility of an edge-on orientation or a lack of prominent spiral arms. No signs of major mergers or strong tidal disturbances are apparent. The overall structure suggests a relatively undisturbed and evolved system.
