The galaxy appears as a faint, elongated structure with a relatively smooth texture. The central region exhibits a slightly brighter concentration of light, suggesting a possible bulge or core. Faint, diffuse extensions are visible from the central region, indicating a disk-like structure with minimal spiral arm definition. The galaxy shows an overall bluish tint, possibly suggesting the presence of younger, hotter stars and ongoing star formation, although at a relatively low rate. The object's shape appears somewhere between round and elongated. There is some evidence of possible disturbances within the galaxy's morphology, however, signs of a major merging event are not apparent.
