The galaxy presents as a generally smooth, elongated structure, suggestive of a disk galaxy seen edge-on. It exhibits a central bulge, which appears to be a reddish hue, possibly indicating an older stellar population with less active star formation in that region. The outer regions of the galaxy display a bluer color, hinting at the presence of younger, hotter stars and ongoing star formation activity. The overall morphology suggests a galaxy that is not currently undergoing significant merging activity, though some minor disturbances may be present in the disk structure. The galaxy's shape is cigar-like with its length appearing roughly 2-3 times greater than its width.
