This galaxy presents as a somewhat elongated, disk-shaped structure, indicative of a spiral or lenticular galaxy viewed at a steep angle. The central bulge appears relatively small and indistinct, suggesting a possibly late-type spiral or an early-type lenticular galaxy. The disk exhibits a smooth texture, lacking prominent spiral arms or distinct star-forming regions. The light profile appears even and there is no indication of significant dust lanes or patchy extinction across the disk. The galaxy has a redder hue, implying an older stellar population with lower levels of ongoing star formation. There are no visually apparent signs of any major interactions or recent mergers. 
