The observed galaxy presents as an edge-on spiral with a prominent disk. The dust lane is extensive and relatively well-defined. The central bulge appears elongated and possibly boxy, with a reddish hue. The disk appears to extend further on one side compared to the other. There is a noticeable concentration of light just outside the central bulge on one side, suggesting a possible region of active star formation or perhaps a satellite galaxy interaction. The overall color profile suggests ongoing star formation, particularly evident from bluer light emanating from the outer regions of the disk. There is no readily apparent evidence of a recent major merger, however there are signs of minor disturbances or interactions.
