The galaxy presents a distinct, elongated morphology, appearing as a cigar shape. The central bulge exhibits a yellowish-orange hue, suggesting an older stellar population likely dominated by evolved stars. Fainter blue regions are observed toward the edges of the galaxy, hinting at more recent star formation occurring in the outer disk. No signs of major mergers or significant tidal disturbances are immediately apparent. The overall smoothness of the light distribution indicates it may be a relatively undisturbed system.
