The galaxy presents as an edge-on spiral. A prominent central bulge exhibits a yellowish-orange hue, suggesting an older stellar population. Extending outward from the bulge is a flattened disk, appearing as a faint, blueish-white band. The dust lane is not clearly visible, but is expected to be obscuring a portion of the central bulge, based on the galaxy's inclination and composition. The overall structure is relatively smooth and undisturbed, with no obvious signs of major mergers or tidal interactions. The blueish tint in the outer regions of the disk may indicate ongoing star formation. The galaxy appears moderately massive and exhibits a moderate rate of star formation, based on its size and color.
