The galaxy presents as an elongated, disk-shaped structure, viewed nearly edge-on. There is a central bulge with high luminosity, suggesting a concentration of older stars. The disk appears relatively smooth, without prominent spiral arms. Coloration suggests ongoing star formation, as evidenced by the bluish-white hue. The light distribution across the disk is not perfectly uniform; it varies slightly along its length. There is an absence of clear signs of tidal disturbances or interactions with other galaxies. It is a relatively isolated galaxy.
