The galaxy presents an elongated, somewhat cigar-shaped morphology, lacking prominent spiral arm structures. It exhibits a smooth, centrally concentrated luminosity profile, suggesting a dominant bulge component. The central region appears brighter and potentially yellower in color compared to the outer regions, which show bluer hues. The overall color gradient indicates ongoing or recent star formation in the outer regions. No obvious signs of major mergers or tidal disturbances are visible, though subtle asymmetries may hint at minor interactions.
