The galaxy presents as a disk galaxy, viewed nearly edge-on. A prominent central bulge is visible, appearing reddish-orange in color, suggesting an older stellar population with diminished ongoing star formation. Faint blue hues are observed along the outer edges of the disk, which suggests the presence of younger, hotter stars and regions of recent or ongoing star formation. The galaxy exhibits a smooth overall structure with no obvious signs of major disturbances or mergers. Subtle irregularities are observed, indicating minor disturbances. The shape of the galaxy is elongated, and the disk appears thin.
