This galaxy exhibits a generally elliptical morphology, with a pronounced cigar shape. Its light profile appears smooth, displaying a concentrated central bulge. The galaxy appears to be dominated by older stellar populations, indicated by the reddish-yellow hue observed throughout. There is no discernible spiral arm structure or significant dust lane obscuration. Faint irregularities or minor disturbances may be present in the outer regions, but they are not prominent enough to suggest a major ongoing merger event. The overall structure indicates a relatively evolved system.
