The galaxy presents as a centrally concentrated elliptical morphology, exhibiting a smooth light distribution with a high degree of circularity. There is no discernible spiral arm structure or bar. The color gradient suggests a population of older stars dominating the galaxy's stellar content, as evidenced by the redder hue concentrated in the core. A gradual decrease in surface brightness is observed as one moves radially outward from the center. There are no obvious signs of recent major mergers or tidal disturbances. Low levels of ongoing star formation activity appear present. Overall, this galaxy appears to be a relatively relaxed, evolved system.
