The galaxy presents as a flattened, cigar-shaped form, elongated along its major axis. A central bulge, appearing relatively smooth and concentrated, exhibits a brighter, more uniform luminosity. The disk component shows some evidence of structure, with subtle variations in color and brightness. The bluer hues, particularly at the periphery of the disk, suggest regions of ongoing star formation. Faint reddish patches can also be seen at the edge of the disk. There is no definitive evidence of a strong bar structure or spiral arms from this view. There does not appear to be a major ongoing merger, although some minor disturbance may be present. Overall, the galaxy appears to be a relatively quiescent system with a moderate level of star formation.
