This galaxy presents as a spiral galaxy, viewed nearly edge-on. It exhibits a prominent central bulge that appears bright and concentrated, displaying a yellowish hue, likely indicating an older stellar population. The disk is also visible but difficult to distinguish. The galaxy appears relatively undisturbed, with no obvious signs of a major ongoing merger. Faint blueish patches are present, likely areas of active star formation within the disk. The galaxy's overall luminosity is considerable, suggesting a substantial stellar mass.
