The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a bright, yellowish core, which likely indicates a high concentration of older stellar populations. There's a gradual decrease in luminosity moving outwards from the center, forming a somewhat diffuse halo. Although a slight asymmetry is observed, there isn't any strong evidence of significant spiral arm structures or prominent dust lanes. The galaxy appears to be largely undisturbed, with no obvious signs of recent major merger events.
