The galaxy presents as a moderately inclined, disk-shaped system. Its overall structure suggests it is a spiral galaxy viewed nearly edge-on. A faint bulge is present, appearing centrally concentrated and diffuse. The disk shows subtle color variations, with a bluer hue, particularly towards the edges, indicating the presence of younger stellar populations and active star formation. Dust lanes appear subtly and sporadically along the disk, attenuating light. No prominent spiral arm structures are distinctly visible in the image, which may be due to the inclination and image resolution. The lack of apparent strong tidal features suggests the galaxy is relatively isolated, with no recent major mergers or interactions disturbing its overall structure. It is likely a galaxy of intermediate mass.
