The galaxy presents as a disk galaxy, observed at a high inclination, appearing cigar-shaped. The central bulge is prominent and exhibits a yellow-white hue, suggesting an older stellar population. The disk itself appears smooth and relatively featureless, lacking distinct spiral arm structures. The outer regions of the disk fade gradually, indicating a decrease in stellar density with increasing radial distance. The overall color of the disk is a slightly bluer shade of white, possibly indicative of a younger stellar population than the central bulge. There is no evidence of significant dust lanes or active star formation regions visible in the image. The galaxy appears relatively isolated, without obvious signs of tidal interactions or ongoing mergers with other galaxies.
