The galaxy presents as a somewhat elongated, spindle-shaped structure, suggesting an edge-on or highly inclined disk galaxy. The central region exhibits a concentrated brightness, indicating the presence of a bulge. A subtle color gradient is observed, with the central bulge appearing more yellowish-orange, possibly indicative of an older stellar population or dust obscuration. Fainter, bluish hues are visible towards the outer regions, hinting at younger, hotter stars and ongoing star formation in the disk. The galaxy appears relatively undisturbed, with no obvious signs of a recent major merger or tidal interactions. Overall, the galaxy appears as a relatively massive spiral galaxy with moderate levels of star formation.
