The galaxy presents as a cigar-shaped system with a smooth light distribution. A central bulge is not readily apparent, suggesting it may be either absent, small, or obscured by dust. The galaxy's light exhibits a gradient, being brighter and more concentrated toward the center, fading gradually towards the edges. The galaxy has a bluer hue around the edges and a redder hue in the center, indicative of different stellar populations and potentially ongoing star formation in the outer regions and an older population in the core. Faint irregularities or disturbances appear present within the galaxy's structure, possibly the result of minor gravitational interactions. There isn't a clear spiral arm structure. The galaxy does not appear to be undergoing a major merger.
