The galaxy presents as a flattened, elongated structure, viewed nearly edge-on. A prominent central bulge is visible, exhibiting a smooth, concentrated luminosity gradient. The disk appears relatively thin and featureless, with only subtle variations in surface brightness along its length. There is a slight indication of dust lane obscuration bisecting the bulge along the major axis. The overall color of the galaxy is skewed toward the redder end of the spectrum. No distinct spiral arm structure or prominent star-forming regions are discernible in this image. The general morphology suggests a disk galaxy, likely of late-type classification based on the edge-on orientation and the presence of a dust lane. There is no apparent evidence of any major ongoing merger events, though minor disturbances cannot be ruled out. The lack of blue regions suggests a low star formation rate.
