The galaxy presents as a flattened elliptical, observed nearly edge-on from our line of sight. A bright, concentrated central bulge dominates the galaxy's structure, exhibiting a yellowish-white hue, suggesting an older stellar population. The surrounding disk appears fainter and more diffuse, with subtle extensions or tidal features present at either end of the major axis. These faint extensions could indicate past minor merger events or tidal interactions. The overall color gradient suggests a radial variation in stellar populations, with the bulge likely being more metal-rich than the outer regions of the disk. There is a very slight blueish tint to the edges. There is no obvious dust lane. The galaxy appears relatively isolated, with no immediately apparent signs of ongoing major interactions or merging activity, although minor disturbances cannot be ruled out.
