The galaxy presents as a relatively luminous, disk-shaped system, observed nearly edge-on from our vantage point. It exhibits a prominent central bulge that appears smooth and elongated along the major axis. The bulge displays a yellowish-orange hue, suggesting an older stellar population and minimal ongoing star formation. The disk component of the galaxy extends outward from the bulge, characterized by a reddish tint. This may indicate a lower rate of star formation in the disk compared to galaxies with bluer colors. There are some signs of slight tidal disruption or minor merging activity in the galaxy. Overall, the galaxy appears to be a fairly massive system with a suppressed specific star formation rate, likely a late-type spiral or lenticular galaxy.
