The galaxy presents as a relatively small, edge-on system. A central bulge is not obviously visible, but a slight brightening in the central region suggests it may be present. The disk appears elongated and quite thin, exhibiting a smooth morphology with no distinct spiral arm structures readily apparent. The galaxy displays a gradient in color, with the inner regions appearing more yellowish-white, transitioning to a bluer hue towards the outer edges of the disk. The overall impression is that of a quiescent, possibly low-mass system, with ongoing star formation primarily located in its periphery. The apparent tilt of the galaxy along our line of sight complicates detailed analysis of its internal structures.
