The galaxy presents as an edge-on or highly inclined disk system. A central bulge is visible, exhibiting a relatively smooth texture and a yellowish hue, suggesting an older stellar population. The disk component appears thin and elongated, with a noticeable dust lane bisecting the galaxy along its major axis, obscuring the light from stars behind it. The disk shows a bluer color gradient compared to the bulge, hinting at ongoing star formation within the disk. No significant spiral arm structure or other prominent features are immediately apparent, given the edge-on orientation. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or major mergers. There is no strong evidence of active galactic nucleus activity visible in this image. Overall, it appears to be a fairly massive, star-forming disk galaxy observed at cosmological distance.
