This galaxy presents an elongated morphology, appearing as a flattened disk viewed edge-on or at a high inclination. A central bulge is weakly apparent, exhibiting a brighter concentration of light relative to the disk. There appears to be a dust lane obscuring a portion of the central regions, creating a dark band across the disk. The disk is composed of a generally smooth light distribution, with little evidence of defined spiral arms or distinct star-forming regions. Based on color gradients, the inner regions appear bluer compared to the outer regions. Overall, the galaxy appears relatively undisturbed with no signs of major mergers or tidal features. Faint, localized disturbances cannot be ruled out.
