The galaxy presents as an edge-on spiral. The primary structure appears to be a flattened disk, exhibiting a high degree of inclination relative to our line of sight. A prominent dust lane is suspected. The central bulge appears relatively smooth and moderately concentrated. The galaxy exhibits a blueish hue, potentially indicative of ongoing star formation within the disk, with a slight reddening towards the central bulge. The galaxy's shape is elongated, with a major axis considerably longer than its minor axis, indicative of a thin disk structure. There is likely a high probability that it is a disk galaxy, as it appears smooth. No obvious signs of strong tidal disturbances or interactions with other galaxies are observed in this image.
