The galaxy presents as an edge-on spiral with an apparent flattening of the disk. A central bulge is discernable, exhibiting a smooth profile. The dust lane appears prominent, bisecting the galaxy. The disk is relatively well-defined, showing a slight asymmetry in its radial extent, with one side appearing more truncated than the other. There is a faint bluish hue concentrated along the outer edges of the disk, suggesting ongoing star formation within the spiral arms. The overall color profile indicates a mix of stellar populations, with a yellower central region and bluer periphery. The galaxy displays no obvious signs of major interaction or recent merger events, although there may be subtle disturbances within the disk suggestive of minor interaction or internal dynamics.
