The galaxy presents as a relatively smooth, centrally concentrated object. The light profile appears to be largely featureless, suggesting an elliptical morphology or a spiral galaxy seen face-on with minimal visible spiral arm structure. The color gradient indicates a concentration of older stellar populations towards the core, as evidenced by the yellow-red hue, which is characteristic of evolved stars. A faint, diffuse halo may be present, but the image resolution limits definitive conclusions regarding its extent and structure. The galaxy shows no obvious signs of ongoing major mergers or tidal disturbances, although minor asymmetries cannot be ruled out with the available data. Based on the observed morphology and color, the galaxy is potentially a quiescent or passively evolving system.
