This galaxy presents as an elongated, edge-on spiral system. A concentrated central bulge is visible, appearing more luminous with a yellowish-orange hue, indicative of an older stellar population likely dominating the bulge. The disk component is noticeably flattened and extends beyond the central bulge. Although the disk is oriented edge-on to our line of sight, it's possible to resolve what may be dust lanes along the plane, appearing as subtle dark bands within the broader structure. The overall morphology suggests a disk galaxy with no indications of major mergers or strong tidal disturbances. However, subtle minor disturbances cannot be completely ruled out. The galactic bulge is rounded, and appears to be more luminous compared to the bluer disk component, which trails away from the bulge.
