The galaxy presents as a lenticular or edge-on spiral, exhibiting a significantly elongated, cigar-like shape. Its overall structure appears smooth, lacking prominent spiral arm features or distinct morphological irregularities, suggesting a high degree of rotational symmetry. The color gradient indicates a central bulge with older stellar populations, reddened by dust, transitioning towards fainter, bluer outer regions, consistent with ongoing but potentially reduced star formation activity. There is no sign of major mergers or tidal disturbances in the image, although it is impossible to say there isn't a smaller ongoing merger. Dust lanes appear minimal or non-existent within this resolution. Overall, the morphology suggests a galaxy evolving toward a more quiescent state.
