The galaxy presents a smooth, centrally concentrated morphology. It exhibits a slight ellipticity, appearing more "in between" round and cigar shaped, rather than perfectly circular. The central region displays a reddish hue, possibly indicating an older stellar population. Surrounding this core is a broader, fainter halo with a blue-green tint. This suggests the presence of younger stars and ongoing star formation, albeit at a low rate. There is no apparent evidence of significant disturbances, tidal tails, or other signs of recent mergers or interactions. The galaxy appears relatively isolated and undisturbed.
