The galaxy presents an elongated, cigar-like morphology, suggesting an edge-on or highly inclined disk. Its central region appears brighter and more concentrated, exhibiting a yellowish-white hue. Fainter, bluish extensions are visible towards the edges of the galaxy, particularly along its major axis. These regions indicate the presence of younger stellar populations and possibly ongoing star formation. The disk appears relatively smooth, with a subtle amount of substructure. There is no evidence of major mergers or significant tidal disturbances, indicating a relatively quiescent evolutionary history. The galaxy appears to be a spiral galaxy of type SBc.
