This galaxy presents as an elongated, disk-like structure with a smooth, centrally concentrated bulge. The central region exhibits a reddish hue, potentially indicating an older stellar population or dust obscuration. Moving outward from the core, the disk shows a transition to greenish and bluish tones, suggesting the presence of younger, hotter stars and/or ongoing star formation in the outer regions. The disk's morphology is relatively smooth, lacking prominent spiral arm structures. The overall shape leans toward a cigar-like appearance, indicating a significant ellipticity. There is no visible evidence of major mergers or tidal disturbances, although subtle asymmetries might suggest minor interactions.
