The observed galaxy exhibits a spiral morphology, though the disk appears to be slightly inclined relative to our line of sight. It demonstrates a prominent central bulge that diminishes gradually into a less dense galactic disk. Faint spiral arms are present; the winding appears generally open or loose, and there is an indication of a two-arm structure. There are no obvious signs of significant tidal disruption or ongoing major merger events. The galaxy's color profile suggests a mix of stellar populations within both the bulge and disk, with a general yellow tone. The relative brightness of the galaxy indicates that it is a substantial galaxy, in terms of both size and stellar mass.
