The galaxy appears to be an elongated, likely spiral galaxy viewed at a steep angle. The central bulge exhibits a yellowish hue, suggesting an older stellar population. Fainter, bluish regions extend from the central bulge, implying ongoing star formation within the spiral arms. The morphology leans towards a smooth appearance, but there is some indication of disc features. The galaxy doesn't exhibit any obvious signs of major mergers or significant tidal disturbances.
