The galaxy presents as a disk galaxy, observed nearly edge-on. The disk appears elongated, with a prominent central bulge. The bulge exhibits a yellowish hue, possibly indicative of an older stellar population. A faint reddish band traces the galactic plane, and some faint blue patches are observed. These indicate regions of potential star formation. No substantial signs of recent major merger events are readily apparent. There are some suggestions of minor tidal disturbances but no substantial evidence of a major recent merger. The general morphology supports a galaxy with a relatively high stellar mass and moderate star formation activity, indicative of a system undergoing relatively steady and stable evolution.
