The galaxy presents a flattened, disk-like morphology. It is oriented approximately edge-on relative to our line of sight. There is a pronounced central bulge region that appears yellowish, suggesting an older stellar population. The disk itself shows a faint bluish tinge, possibly indicating regions of recent or ongoing star formation. It appears relatively smooth with no distinct spiral arm structure readily discernible at this resolution, potentially due to the viewing angle. The galaxy shows a slight asymmetry, with a somewhat elongated shape. There is no clear evidence of a major ongoing merger or significant tidal disturbances, though a subtle asymmetry may imply a minor interaction or past interaction with another object.
