The galaxy appears as a relatively smooth, elongated object, possibly disc-like, with a bright central bulge. It has a distinctly cigar-shaped morphology. The light profile seems relatively smooth, with no immediately obvious spiral arm structures, though some subtle asymmetry is present. The color distribution suggests a higher concentration of older stellar populations in the central region, indicated by the yellowish hue, transitioning to bluer tones in the outer regions, possibly indicating more recent star formation. There are signs of minor disturbances in the galaxy's structure. Overall, the galaxy appears to be an evolving system experiencing moderate star formation activity.
