The galaxy presents as an elongated, disk-shaped structure viewed nearly edge-on. There is a central bulge that appears relatively prominent. The color distribution shows a concentration of yellow/red light toward the bulge, suggesting an older stellar population dominating that region. The outer disk exhibits a bluer hue, possibly indicating ongoing star formation, even if at a low rate. The disk appears smooth and relatively undisturbed, showing no signs of strong tidal interactions or major merger events. There is a slight suggestion of a boxy structure to the bulge. The absence of readily visible dust lanes is notable given the edge-on orientation.
