The galaxy presents as a relatively smooth, disk-shaped object, oriented approximately edge-on with respect to our line of sight. A bright, centralized bulge dominates the core region, exhibiting a yellowish-white luminosity suggesting an older stellar population. Circumferencing the bulge is a more diffuse disk, showing a slight bluer hue indicating ongoing star formation within spiral arm structures that are not distinctly resolved. There's a faint reddish tint within the disk, possibly indicating the presence of dust lanes or regions of intense star formation obscured by dust. Faint asymmetry along the galaxy, may suggest minor gravitational interactions with a nearby galaxy.
