The galaxy presents as an edge-on spiral. A prominent central bulge appears yellowish-orange, suggesting an older stellar population and lower star formation rate within this region. The disk is visible as a flattened structure extending outwards from the bulge, displaying a blueish hue likely due to the presence of younger, hotter stars and ongoing star formation. The galaxy's morphology appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. The bulge seems to have a rounded shape. The galactic disk appears smooth. Overall, it presents the characteristics of a well-formed, relatively quiescent spiral galaxy.
