The galaxy presents as a lenticular or edge-on spiral, exhibiting a distinct flattened disk structure. The central bulge appears relatively prominent, with a bright, concentrated luminosity profile indicating a significant stellar population. The disk displays a smooth texture and is elongated with an aspect ratio suggesting a high degree of inclination relative to our line of sight. There is an asymmetrical distribution of bluer, diffuse light along the disk, possibly indicating recent or ongoing star formation regions, especially towards one end. The overall color is moderately blue-shifted, suggesting a population of young to intermediate age stars throughout the galaxy. There's little evidence of tidal features or interactions with neighboring galaxies, suggesting that the galaxy is relatively isolated and quiescent. No distinct spiral arms or dust lanes are immediately visible.
