The galaxy appears as a moderately bright, disk-shaped object. It exhibits a relatively flattened profile, suggesting it may be viewed at an angle that is not quite edge-on. The central region of the galaxy is characterized by a brighter, concentrated area, likely indicative of a bulge component. Surrounding the central bulge, a disk is visible, showing a hint of spiral structure, though details are somewhat obscured. There is some evidence of possible interaction or disturbance in its morphology, particularly at the outer edges of the disk, which appear slightly irregular or extended. Color gradients are present, with the central bulge appearing to be a yellowish color, possibly indicating an older stellar population, while the disk appears somewhat bluer, suggesting the presence of younger stars or ongoing star formation. The overall light distribution seems to be smooth, although some patchy regions may be present within the disk. The faintness and lack of clearly defined features may indicate the galaxy is distant.
