The galaxy presents a generally smooth appearance with a distinct elongated, cigar-like morphology. The primary color is a light blue or cyan hue, suggesting the presence of younger stellar populations and some ongoing star formation, albeit perhaps at a relatively low rate. The overall structure lacks prominent spiral arms or a defined central bulge, giving the impression of a disk galaxy viewed at a high inclination. There is no strong evidence of any major merger events, but some minor disturbances or asymmetries within the galaxy's structure cannot be ruled out based on the current image resolution. The galaxy appears relatively isolated with no obvious companion galaxies in close proximity. 
