The galaxy presents as an elongated, spindle-shaped structure. It displays a smooth, diffuse morphology with a central, brighter core region that appears somewhat concentrated. The overall color profile suggests a reddish-yellow hue, possibly indicating an older stellar population with less active star formation. Faint extensions are observed beyond the brighter core, hinting at a disk-like structure viewed edge-on. There may be some subtle dust lane obscuration although this cannot be confirmed from this imagery. There is no sign of significant mergers or tidal disruption. The galaxy seems relatively isolated. 
