The observed galaxy presents as a moderately inclined spiral with a faint, diffuse appearance. The galaxy exhibits a subtle bluish hue overall, suggesting the presence of younger stellar populations within its structure. Evident within the galaxy is a distinct, albeit somewhat irregular, disk-like component. Subtle variations in the light distribution are detectable within the disk, hinting at the presence of spiral arm features. These arms appear relatively tightly wound.

No pronounced bulge is visible at the galaxy's core. This might mean it's either too faint to detect or the galaxy is a late type spiral. There seems to be a hint of slight asymmetry in the galaxy's overall structure. There may be some signs of a past, minor merger.
